The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The color is predominantly yellow-orange, suggesting an older stellar population with a low rate of ongoing star formation. There is little evidence of spiral arms or a disk-like structure; the light distribution is largely spheroidal. The galaxy exhibits a high degree of symmetry and circularity, implying it is not currently undergoing any major mergers or significant tidal disturbances. There is a slight color gradient with the central region appearing slightly redder, possibly indicative of a higher concentration of older, redder stars towards the core. Overall, the galaxy presents as a well-evolved, quiescent system.
