The galaxy presents a somewhat elliptical morphology, suggesting it is likely an elliptical galaxy. There is a notable central bulge, appearing as a concentrated region of primarily yellowish-white light, indicating an older stellar population in this area. The bulge transitions into a more diffuse outer region. The outer regions exhibit a lower surface brightness than the bulge, presenting a mix of colors, predominantly reddish hues interspersed with hints of bluer tones. The galaxy appears to have a smooth structure, with no obvious signs of spiral arms or significant dust lanes, and no evidence of a strong tidal disturbance or merger. The galaxy has a red shift value, indicating it is in the more distant universe. Overall, the light distribution and structure support a classification as an elliptical galaxy with a developed spheroidal component.
