The galaxy presents as a relatively compact, disk-like structure, exhibiting a pronounced central bulge. It appears to be undergoing some form of interaction, perhaps a minor merger or tidal disruption event. This is evidenced by the slight asymmetry in its overall shape, as well as a faint, wispy extension or tidal tail emanating from one side.

The galactic disk shows minimal resolved structure, suggesting a relatively smooth stellar population. However, there is an indication of some internal dust obscuration along a horizontal band, as shown by a band of blue. The outer regions of the galaxy are less well-defined, with a gradual fading of light intensity towards the surrounding background. A pinkish hue is visible at the center of the galaxy, this is likely attributed to star formation.
