The galaxy presents as a moderately bright, elliptical-like structure with a smooth, centrally concentrated light distribution. Its color profile indicates an older stellar population, with a dominant yellow-red hue in the central bulge, suggesting a lack of ongoing star formation. The galaxy's shape appears to be somewhat elongated. There is a faint disk-like structure surrounding the bulge that is difficult to see and may be an artifact of the image quality. There is no visual evidence of tidal disturbances, mergers, or active star formation regions. The galaxy seems relatively isolated and undisturbed. Overall, it is a mature galaxy, likely consisting of mostly old stars.
