The galaxy presents as a roughly elliptical, moderately compact object. The light distribution is centrally concentrated, with a relatively smooth overall appearance. There is some evidence of a slight elongation, with the major axis oriented roughly vertically.

The color gradient suggests a population of primarily older stars, contributing to the reddish-yellow hue. However, there appears to be a small patch of bluer light, hinting at some ongoing, albeit low-level, star formation. There may be the beginnings of a disk galaxy, as it does not appear perfectly spherical. There is no clear evidence of spiral arm structure.

The galaxy appears to be relatively isolated. There is a second, blue object near the galaxy, but does not appear to be tidally interacting or merging with the galaxy, though it is possible. There is a hint of a disturbance, but is not significant.
