The galaxy appears to be a relatively smooth, elliptical system. The light distribution is concentrated toward the center, indicating a dense nucleus or bulge. The overall shape is quite round, with no obvious disk-like structure or spiral arms visible. There are no major disturbances or signs of ongoing mergers apparent in the image. The galaxy exhibits a subtle color gradient, with the core appearing whiter than the outer regions, suggesting an older stellar population in the central area and possibly some younger stars in the outskirts. There are no distinct tidal tails or streams detected, further supporting the absence of recent major interactions. Overall, the galaxy appears to be a well-formed, relaxed elliptical galaxy.
