The galaxy presents as a relatively small, well-defined elliptical shape with a noticeable disk-like component. The central bulge appears bright and yellow, suggesting a population of older stars. A faint disk, seen nearly edge-on, is oriented horizontally through the center of the bulge. The disk exhibits a bluer hue, indicating the presence of younger, hotter stars, potentially associated with ongoing star formation. The galaxy does not appear to be undergoing any major merger activity, though some minor disturbances or tidal features cannot be entirely ruled out. Overall, the galaxy exhibits a smooth, rounded morphology, consistent with an early-type spiral or lenticular galaxy at a moderate redshift.
