The galaxy presents as a relatively smooth, elongated object. It is likely an elliptical galaxy viewed at an angle. The core of the galaxy shows a concentrated luminosity, gradually fading into the outer regions. The color profile seems to show a dominance of older stellar populations with faint bluish concentrations that are interspersed throughout. There is no definitive evidence of a spiral structure, although subtle disturbances may be present, not indicative of a major merger. The galaxy appears relatively isolated, with no immediately apparent tidal features or close companions that would suggest recent or ongoing interactions.
