The galaxy presents as a somewhat symmetrical, centrally concentrated object with a noticeable, yet not highly pronounced, bulge region. The overall shape is somewhat round, though with some slight deviation from perfect circularity.

The color profile suggests a dominant older stellar population. There is a relatively small amount of bluer light observed, suggesting some ongoing, but not intense, star formation.

The galaxy appears relatively isolated, without obvious signs of major tidal disturbances or interactions with other galaxies, though there is what appears to be a smaller galaxy located nearby. No dust lanes or other distinct features are readily apparent in this image. The galaxy's core appears smooth and well-defined.
