The galaxy presents as a moderately luminous, relatively smooth, and somewhat elongated structure. Its color profile suggests a dominant population of older stars, indicated by the yellowish hue concentrated in the central bulge, but there is also evidence of a faint blueish disk. The morphology is generally elliptical, although there may be a slightly flattened disk component. There is no obvious spiral arm structure or signs of significant recent star formation. No apparent major mergers or tidal disturbances are observed. The galaxy appears to be relatively isolated, showing no strong gravitational interactions with nearby galaxies.
