The galaxy presents as a relatively compact object with a smooth, centrally concentrated luminosity profile. There is minimal evidence of spiral arm structure or a distinct disk. The overall shape appears to be generally elliptical, trending towards a more rounded morphology, though slight elongation cannot be ruled out.

The galaxy exhibits a range of colors, with the central region displaying a brighter, bluer hue that transitions to redder tones in the outer regions. The bluer core potentially suggests ongoing star formation or a significant population of younger stars. There is no obvious evidence of a major merger event; however, the galaxy's morphology could potentially reflect a past minor disturbance or interaction. The galaxy appears relatively isolated in its immediate environment.
