The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated luminosity profile, with brightness decreasing gradually from the core towards the outer regions. There is a slight elongation to the overall shape, suggesting it is not perfectly spherical, trending towards a cigar shape. The color distribution appears fairly uniform across the galaxy, though the central region appears somewhat redder and brighter than the outer disk, implying a relatively homogenous stellar population. There is little evidence of spiral arm structures or prominent dust lanes. The edges of the galaxy are ill-defined, fading gently into the background sky without sharp boundaries, indicative of an absence of ongoing star formation. There is a hint of a minor disturbance in its form, possibly indicating a past or ongoing interaction with a smaller galaxy.
