The galaxy presents as a slightly elongated, cigar-shaped structure. Its light is dominated by warmer hues suggesting an older stellar population, with a concentration of yellowish-orange light towards the central region, indicating a likely bulge. The outer edges appear fainter and bluer, hinting at some ongoing, albeit limited, star formation within its disk. There is no clear spiral structure visible. The overall morphology suggests an elliptical or lenticular galaxy with an estimated size of approximately 9 kpc. There is no readily apparent evidence of any major ongoing merger activity or significant tidal disturbances. The structure appears relatively smooth, but possible minor interactions cannot be ruled out, as there are some irregularities.
