The galaxy presents as a slightly elongated, disk-like structure. It exhibits a bright, concentrated central bulge, which appears yellowish in color, possibly indicating an older stellar population. The overall luminosity suggests a significant stellar mass.

A faint, bluer disk surrounds the bulge, hinting at ongoing star formation. The disk's structure appears relatively smooth, with minimal visible spiral arm features or dust lanes. There's a very slight disturbance in the disk on the left side. The shape is more in between round and cigar shaped.

The general morphology of the galaxy indicates it's not currently undergoing a major merger event, though there are some hints of minor disturbances.
