This galaxy appears to be an elliptical type, characterized by a generally smooth and featureless morphology. It has a concentrated central bulge region exhibiting a yellowish-orange hue, suggesting an older stellar population and lower levels of ongoing star formation. The isophotes appear relatively round, indicating a low degree of ellipticity. Faint, diffuse blue light surrounds the central bulge, which may indicate the presence of a very faint disk. There is no obvious tidal debris, close companions or morphological distortion, suggesting the galaxy has not recently undergone a major merger event. Overall, this galaxy presents as a mature, isolated system.
