The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular type. The central region exhibits a concentrated brightness, possibly indicating a substantial galactic nucleus. A slight elongation is observed, deviating from a perfectly circular shape, which could indicate a mild interaction or intrinsic asymmetry. Color gradients within the galaxy show a redder hue in the central region that transitions to a slightly bluer one towards the outer edges. A secondary, smaller object with a reddish color is located close to the primary galaxy, which may be a satellite galaxy, however, it is difficult to determine if it is interacting with the primary galaxy or not. There does not seem to be a massive amount of star formation going on.
