The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a notable absence of distinct spiral arm structures or prominent dust lanes. The overall color profile leans towards the redder end of the spectrum, indicative of an older stellar population, although there may be a small amount of recent star formation. The light is generally uniformly distributed, with no significant evidence of tidal tails, strong asymmetries, or active galactic nucleus features apparent in this image. The galaxy appears generally isolated with some evidence of a possible merger occurring in the past. The shape is consistently round. The galaxy exhibits a moderate size, as determined by its estimated half-light radius.
