This galaxy presents as a roughly elliptical, though somewhat irregular, structure. The central region exhibits a concentrated luminosity, suggesting a dense stellar population. Extending outwards, the luminosity gradually diminishes into a more diffuse halo. Some features might be interpreted as tidal tails or signs of an ongoing or recent merger event, specifically between two components, or some form of minor galactic disturbance. The overall color suggests a predominantly older stellar population, though there may be localized regions of relatively more recent star formation activity, implied by subtle variations in color. The galaxy's apparent shape deviates from a perfect ellipse and presents as cigar-shaped, suggesting it is not viewed directly face-on. There may be some minor dust lanes that obscure sections of the light coming from the body of the galaxy.
