The galaxy appears to be a relatively smooth, elliptical or lenticular type galaxy. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. The color profile suggests an older stellar population, with the central region displaying a yellowish-orange hue consistent with older, redder stars. There is little evidence of active star formation, as indicated by the lack of distinct blue regions or spiral arm structures. The overall morphology is somewhat elongated, but primarily round, without any signs of ongoing major mergers or significant tidal disturbances. There may be some minor asymmetry or irregularity in the outer halo region, possibly indicative of a past minor interaction or accretion event. The galaxy shows a moderate redshift, placing it at a considerable cosmological distance.
