The galaxy appears to be a relatively smooth, elongated structure. Its color profile leans towards the redder end of the spectrum, with a noticeable lack of distinct blue regions. The morphology suggests it is likely an elliptical galaxy. The primary body of the galaxy exhibits a concentrated central bulge that gradually fades into its outer regions. There is no apparent spiral arm structure or evidence of significant dust lanes. The galaxy displays a fairly uniform texture without any strong indicators of ongoing, large-scale star formation. There is no clear evidence of a major merger event, though subtle signs of tidal disturbances or minor interactions cannot be ruled out. It may possibly be undergoing low rates of star formation.
