The galaxy presents as a single, relatively smooth object. It appears elliptical, with a concentrated central bulge. The core is a strong yellow hue, suggesting an older stellar population, while the outer regions exhibit a more greenish-yellow tint, which might indicate a younger stellar population that is actively forming stars, although this activity seems to be at a moderate level. There appears to be no spiral arm structure or prominent dust lanes visible within the galaxy, and no sign of merging activity or major disturbance. It is mostly round in shape with a very slight elongation.