The galaxy presents as an elliptical or lenticular type, exhibiting a relatively smooth morphology. The central bulge is bright and concentrated, with a blue-white hue, suggesting a population of younger, hotter stars or perhaps a bright active galactic nucleus. A disk-like structure surrounds the central bulge, although it lacks well-defined spiral arms.

The disk displays some evidence of disturbances, possibly due to a minor interaction or past merger event. This is indicated by a faint, somewhat irregular distribution of material.

The overall color profile shows gradients, with the central region appearing bluer, transitioning to more red-shifted tones in the outer regions of the disk. This is indicative of stellar population variations, potentially with older, redder stars dominating in the galaxy's periphery. The galaxy does not appear to be undergoing a major merging event. There may be a small tidal tail or extension on one side, although this needs further investigation to rule out artifacts or background contamination.
