The galaxy presents as an elliptical morphology, though a faint disk-like structure is weakly suggested. The light is notably concentrated toward the center of the galaxy, creating a defined bulge. The color profile indicates an older stellar population. The galaxy exhibits a color gradient transitioning from a yellow hue in the bulge to a somewhat redder appearance in the outer regions. The outer edges are poorly defined, suggesting a gradual fading into the background sky. There is no evidence of active star formation in this image. The general form of the galaxy can be described as cigar-shaped. There is no strong evidence of a major merger or significant tidal disturbance.
