The galaxy appears as a moderately bright, elongated structure. A dominant central bulge is visible, exhibiting a yellowish hue indicative of an older stellar population. There is evidence of a faint disk component, with a bluer color suggesting the presence of younger, hotter stars.  The disk appears somewhat disturbed or asymmetric. There is potentially minor interaction happening with the galaxy to the right of the primary structure. The galaxy's overall morphology suggests a transition stage between an elliptical and a spiral type, or a disk galaxy that has undergone some disturbances.
