The galaxy presents as a relatively smooth, elliptical-like structure with a moderately concentrated light profile. Its overall color is yellowish-red, suggesting an older stellar population with minimal ongoing star formation. There appears to be a slight elongation but nothing suggesting a spiral structure. The main body seems largely undisturbed, however there is a secondary, slightly dimmer, and potentially interacting, galaxy nearby. It's challenging to determine from this image whether this is a true merger or a line-of-sight alignment. The primary object appears round, albeit with a subtle cigar-like quality. There is no significant evidence of tidal tails or shells that might be indicative of a recent major merger event. A more detailed spectral analysis would be needed to ascertain the age and composition of the galaxy.
