The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a brighter, more concentrated luminosity. Moving outward from the center, the light gradually diffuses, and the overall shape appears somewhat elongated, more akin to a cigar shape than a perfect sphere. There is no apparent spiral arm structure or prominent dust lane visible in this image. The galaxy appears relatively isolated with no obvious signs of a major ongoing merger, though there may be some minor disturbances in its form. The color profile suggests a population of older stars.
