The galaxy presents as a generally smooth, elliptical-like structure, though slightly elongated. Its light distribution is concentrated towards the center, exhibiting a bright, somewhat diffuse core region, with color indicative of older stellar populations. Proceeding outwards, the luminosity smoothly decreases into an extended halo with a slight reddish hue, suggesting a population of older, redder stars in this region. There is little evidence of strong spiral arm structure or significant dust lanes. A cigar shaped morphology is evident, suggesting a possible elliptical galaxy undergoing some form of tidal interaction or internal dynamical process that is causing the deformation. There appears to be very mild disturbances present within the shape of the galaxy, such as an irregularity of the shape, however it is difficult to identify any signs of a major ongoing merger event.