The galaxy presents as a relatively smooth, elliptical or lenticular structure, exhibiting a moderately elongated shape. There is a distinct, bright central bulge with a gradual decline in luminosity towards the outer regions. Faint, diffuse features are visible, suggestive of a possible disk or spiral arm remnants, however, these are not well-defined. There is no clear evidence of active star formation regions or significant dust lanes within the galaxy itself. Overall, the galaxy appears relatively undisturbed, without any prominent signs of ongoing major mergers or tidal interactions.
