The galaxy appears to be an elliptical or lenticular type with a smooth, centrally concentrated bulge region. The main body of the galaxy is somewhat elongated. There is a suggestion of a disk component, although it is not well defined, hinting at a transition type. The central region presents a slightly redder hue compared to the more diffuse outer regions, which appear bluer and suggest some degree of recent star formation. There are signs of some minor disturbances in the outer disk indicating possible gravitational interaction with neighboring galaxies. It does not appear to be involved in a major merger. Overall, the galaxy exhibits properties that suggest a moderate stellar mass and moderate ongoing star formation within a relatively compact volume.
