The galaxy appears to be a single, relatively smooth object, lacking prominent spiral arms or a bar structure. It exhibits a centrally concentrated luminosity profile, with the brightest region located in the core. The overall shape is somewhat elliptical, though not perfectly spherical. The color distribution suggests a population of older stars, and there is no indication of recent major merger activity, tidal tails, or strong asymmetries, suggesting it is relatively isolated and undisturbed. There may be minor disturbances but they are hard to discern. The galaxy displays colors consistent with those of an early-type galaxy, though there are some traces of bluer colors that suggest there is some, albeit low, amount of star formation occurring.
