The object appears to be a galaxy, exhibiting a generally smooth morphology. The central region displays a bright, concentrated luminosity, suggesting a significant stellar density and potentially a supermassive black hole at the galactic nucleus. Moving outward from the center, the luminosity gradually diminishes, although a faint, diffuse halo is visible extending beyond the core.

The galaxy exhibits a slight ellipticity, appearing somewhat flattened rather than perfectly spherical. A subtle color gradient is observed, with the core appearing more yellowish, and the outer regions tending toward redder hues. This could indicate a difference in the stellar population, with older, redder stars dominating the outer regions.

There is no obvious spiral arm structure visible in the image. The overall appearance suggests an elliptical galaxy, likely composed of older stars and exhibiting a relatively low star formation rate. There's no evidence of any ongoing major merger events. Subtle asymmetry may be visible in the outskirts, though this is difficult to ascertain given the image quality.
