The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light distribution. The overall shape is elongated, appearing somewhat cigar-shaped rather than perfectly spherical. The color gradient suggests a population of older stars dominating the central regions, indicated by a yellowish hue, while fainter blue-ish regions are seen towards the edges, potentially suggesting a low level of ongoing star formation activity. There is no evidence of spiral arms or a prominent disk structure. No major distortions are visible, suggesting it is not currently undergoing a major merger. A minor disturbance may be present, as there seems to be a very faint and subtle asymmetry.
