The galaxy presents a morphology consistent with an elliptical galaxy, exhibiting a largely smooth and centralized light distribution. The color profile indicates a concentration of older stellar populations, as evidenced by a redder hue concentrated towards the central region, gradually transitioning to bluer hues towards the outer edges. The overall shape is approximately round, with only a slight deviation towards ellipticity. There is a possible minor disturbance in the structure, possibly a small tidal feature or a slight asymmetry, that suggests a past or ongoing interaction. However, there is no strong evidence of a major merger or significant disruption to the overall structure. The lack of well-defined spiral arms or prominent dust lanes further supports classification as an elliptical galaxy.
