The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse appearance. It exhibits a slight elongation, deviating minimally from a perfectly circular form. The core is a bright, compact region, suggesting a high density of stars. The color profile shows a distinct red-yellow hue concentrated in the central region, indicative of an older stellar population. The outer regions display a gradual decline in luminosity, fading into the background sky. No prominent spiral arms or dust lanes are visible. There is no indication of a recent major merger or significant tidal disturbances, though a slight asymmetry in the outermost isophotes cannot be ruled out. The overall morphology is consistent with an elliptical galaxy at a redshift of approximately 0.103. Star formation activity is likely low, as suggested by the colors and smooth morphology.
