The galaxy appears to be a relatively smooth, elliptical system. The light distribution is centrally concentrated, with a noticeable falloff in brightness towards the edges, indicating a lack of prominent spiral arms or distinct features. Its overall shape approximates a circular morphology, exhibiting a slight deviation from perfect roundness. There are no obvious signs of recent or ongoing major mergers or tidal disturbances. The galaxy exhibits a moderate level of star formation, likely indicative of an intermediate population of stars. The color suggests an older stellar population, but with some younger, bluer stars contributing to the overall light. The galaxy has a moderate luminosity.
