The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light profile decreases gradually from the core outwards, suggesting a bulge-dominated system. The galaxy's color is predominantly yellow, with a slight reddish hue, suggestive of an older stellar population and possibly a suppressed star formation rate. There is no evidence of strong spiral arms, prominent dust lanes, or significant ongoing star formation regions visible within the galaxy's disk. The lack of distinct morphological features implies that this is likely an elliptical galaxy or a lenticular galaxy viewed face-on. The relatively round appearance indicates that it is not highly inclined relative to our line of sight. There is no clear sign of any major mergers or tidal disturbances affecting the object's structure, suggesting it is relatively isolated or in a dynamically stable state.
