The galaxy presents as a relatively compact object, approximately circular in overall shape with a slight asymmetry visible on its right side. There appears to be a bright, concentrated central region, possibly indicative of an active galactic nucleus or a dense stellar population.

The galaxy's color profile suggests a bluer hue in the central portion, transitioning to a redder shade towards the outer edges, suggesting that there is ongoing star formation within the inner portion of the galaxy. The outer region's redder color suggests that there are older stars present, or possibly dust obscuring younger, bluer stars. 

A minor disturbance seems to be present on the galaxy's right side, possibly indicating an interaction with a smaller galaxy or tidal effects from a past merger event. Overall, the galaxy exhibits characteristics that suggest it is somewhere between a smooth elliptical type and a disk galaxy with some features. Further analysis is warranted to determine the precise morphological classification and the nature of the observed disturbance.
