The galaxy presents as a disk galaxy, viewed at an oblique angle, but not quite edge-on. The galaxy displays a smooth overall structure, with a bright, concentrated central bulge indicative of a significant spheroidal component. The bulge appears somewhat elongated.

The disk component shows a subtle flattening, with the major axis significantly longer than the minor axis. Evidence of spiral arm structure is not readily apparent.

The color profile of the galaxy suggests a relatively old stellar population, with the bulge exhibiting a yellowish-white hue. The outer disk appears slightly bluer, hinting at the presence of some younger stars and ongoing star formation, but with a relatively low star formation rate. There is no clear indication of any major recent merger events, although a slight asymmetry in the disk could point to a past minor interaction. The galaxy is compact, with a relatively small effective radius.
