The galaxy presents as a largely elliptical morphology, exhibiting a smooth light distribution with minimal discernible features. The central region displays a higher concentration of luminosity, suggesting a prominent galactic nucleus or bulge. Proceeding outward, the light gradually diminishes, revealing a subtle gradient into the less dense outer regions.

In terms of color, the galaxy exhibits a subtle reddish-yellow hue, suggesting an older stellar population. This would indicate that the stars are primarily older, lower mass stars that are evolving off the main sequence. This reddish-yellow tone gradually transitions to a bluer hue in the outer regions. Based on its smooth form and older population, it is unlikely to be undergoing high rates of star formation.

No distinct spiral arms or bar structures are apparent, which would also support its classification as elliptical. There is a very slight irregular feature present indicating minor disturbance through a possible tidal interaction with a small nearby galaxy, or perhaps the last remnant of a past merger.
