The galaxy presents as a relatively concentrated elliptical or lenticular structure. Its light profile appears smooth, with a gradual falloff from the core to the outer regions. The core region is noticeably brighter than the outer disk, with a yellowish-white hue, suggesting an older stellar population dominating the nuclear region. A faint, bluer tinge is visible on the edges of the galaxy, perhaps indicating some ongoing, albeit limited, star formation in the outer regions. The galaxy exhibits a slight elongation in its shape, appearing somewhat flattened. Overall, the galaxy appears to be an evolved system with minimal to no spiral arm structure visible in the image.
