The galaxy presents a primarily smooth, elliptical morphology with a high degree of central concentration. The light profile is centrally peaked, indicating a significant bulge component. There appears to be little to no disk structure, and the overall shape is somewhat elongated but not strongly cigar-shaped. The color distribution is not uniform; the central region exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter bluish regions appear asymmetrically distributed around the central bulge, potentially indicative of recent, albeit low, levels of star formation. There is no discernible evidence of any major mergers or tidal disturbances. The galaxy appears relatively isolated and undisturbed.
