The galaxy appears as a concentrated, luminous object with a generally elliptical morphology. Its central region displays a bright, somewhat diffuse glow, suggesting a concentrated stellar population or an active galactic nucleus. The galaxy’s overall color is skewed towards the redder end of the spectrum, implying an older stellar population, substantial dust obscuration, or significant redshift. There's a slight elongation in its shape but the galaxy is mostly rounded in appearance. There is no obvious spiral arm structure or prominent dust lanes visible. Faint extensions or tidal features are not readily apparent, but the moderate image resolution could obscure subtle details. The galaxy exhibits a relatively smooth profile, indicating a lack of major ongoing mergers or significant star-forming regions. Possible minor disturbances or faint features might exist but cannot be confirmed without higher-resolution data.
