The galaxy appears to be a relatively smooth, elliptical-like structure with a slightly elongated shape. Its color is predominantly a pale blue, indicating a population of younger, hotter stars, although some older, redder stars are likely present, contributing to the overall hue. There is no apparent spiral structure or distinct dust lanes. The galaxy exhibits a fairly concentrated central bulge, with the light intensity gradually decreasing towards the edges, forming a diffuse halo. There is no evidence of significant tidal disturbances or ongoing major mergers. Overall, the galaxy seems to be in a relatively quiescent state.