The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a bright, concentrated core, indicative of a substantial stellar population. The light profile decreases steadily from the core outward, suggesting a lack of distinct spiral arms or other prominent features. The galaxy appears to be somewhat spheroidal in shape, lacking any significant elongation. There is no evidence of major disturbances or ongoing merger activity, although subtle asymmetries in the outer regions might suggest minor interactions in the past. The overall color appears to be consistent with an older stellar population, dominated by redder wavelengths. The size is consistent with it being a smaller galaxy.
