The galaxy presents a generally smooth, elliptical morphology. Its color index, assessed visually, suggests a population of older stars, contributing to a redder overall hue. There is minimal apparent dust obscuration and no indications of significant spiral arm structure. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or recent mergers, though a slight asymmetry may be present, meriting further investigation. The central region exhibits a gradual increase in surface brightness towards what appears to be a concentrated core. The estimated physical size of the galaxy is on the order of several kiloparsecs, indicative of a moderate-sized system. Analysis of its spectral properties is likely to reveal relatively low levels of ongoing star formation. The galaxy is fairly round in shape.
