The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light distribution appears centrally condensed with a fairly rapid fall off in intensity from the core towards the outer regions, suggesting an older stellar population. While there is some subtle color variation across the galaxy, it does not exhibit strong spiral arm structures or prominent dust lanes. The overall color appears yellowish, which further supports the inference of an older stellar population and potentially lower levels of ongoing star formation. There is a slight asymmetry in the galaxy's shape, but it does not appear to be undergoing a major merger, though minor disturbances cannot be ruled out.
