The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape. The central region exhibits a bright, concentrated luminosity, suggesting a substantial stellar density, potentially indicative of an older stellar population. Moving outward, the light intensity gradually diminishes, with a diffuse halo extending beyond the bright core. There is no apparent disk structure or spiral arm features visible. No prominent dust lanes or regions of active star formation are discernible based on the image. The galaxy appears relatively isolated, showing no clear signs of tidal interactions or major disturbances in its structure. Overall, the galaxy appears to be a relatively massive and well-evolved system.
