The galaxy presents as a relatively smooth, centrally concentrated object. The overall morphology appears elliptical, exhibiting a high degree of roundness with only subtle deviations from a perfect circle. A bright central bulge is visible, gradually fading into a diffuse halo. Some subtle signs of faint, disturbed features, such as slight asymmetries, are present, suggesting possible tidal interactions or minor merger events in the galaxy's past. In general, no strong spiral arm structures or distinct dust lanes are observed, in line with its smooth appearance. The galaxy's color profile indicates a population of older stars.
