The galaxy presents an overall elliptical morphology, appearing moderately elongated rather than perfectly spherical. Its core exhibits a concentrated luminosity, suggesting a dense stellar population or potentially an active galactic nucleus. The light profile fades gradually from the center, indicating a smooth distribution of stars. Some subtle structures are visible with areas of patchy color variation. The galaxy's color is predominantly yellowish-white, with possible hints of bluer regions in the outer edges, indicating the presence of some younger, hotter stars mixed with a larger population of older stars. There are areas of minor disturbance in the morphology, possibly indicating interaction with another galaxy, though it does not appear to be a significant merger event. There is some evidence of tidal tails or extended debris.
