The galaxy presents as a relatively smooth, centrally concentrated object. It appears nearly circular in shape with a dominant, bright central bulge region, which suggests a significant population of older stars. There is a subtle colour gradient visible, with the central region exhibiting a slightly redder hue compared to the outer regions, which show hints of bluer light. This could be attributed to recent or ongoing star formation in the outer regions, or could simply be a result of dust obscuration. No obvious spiral arms or bar features are discernible. There is no obvious indication of a major ongoing merger. The galaxy shows minor disturbances. The galaxy has an estimated size of approximately 4 kpc in radius. The overall appearance points to a relatively evolved system.
