The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an overall elliptical morphology, appearing largely spheroidal in shape without prominent spiral arm structures or a distinct disk component visible in this observation. A color gradient is apparent, with the central region displaying a reddish hue, suggestive of an older stellar population. The outer regions exhibit a bluer color, which may indicate the presence of younger stars or ongoing star formation, although this is not obviously pronounced. There is a marginal indication of some disturbance in the galaxy's form, but no evidence of any major ongoing merger. The light is gradually diminishing from the center. The galaxy's physical extent is considerable and roughly ~12 kpc in radius. Overall, the galaxy appears to be relatively massive and undergoing a low level of star formation.
