The galaxy exhibits a smooth, elliptical morphology. The central region is notably brighter and appears yellowish, indicating an older stellar population. Moving outwards from the core, the color transitions to a slightly bluer hue, suggesting the presence of younger stars, although the overall star formation rate appears relatively low. The galaxy lacks prominent spiral arms or a distinct disk structure. There is a very subtle asymmetry in the outer regions. There is no indication of any major or minor disturbances from recent merging activity. The galaxy appears to be in a relatively relaxed state.
