The galaxy appears to be a relatively smooth, elliptical type, displaying a yellowish central bulge. The light distribution suggests an older stellar population, with less evidence of ongoing star formation in the central region. There is a slight elongation along one axis, suggesting a deviation from a perfectly spherical shape, but it does not appear to be highly flattened. No prominent spiral arms, dust lanes, or tidal features are readily apparent, indicating it is likely an isolated galaxy that hasn't recently undergone a major merger. Faint, diffuse blue light extending from the central region hints at the possibility of some residual star formation in the outer regions of the galaxy.
