The galaxy presents as a slightly elongated, lenticular structure. Its morphology suggests a relatively smooth profile with a bright central bulge that fades gradually towards the edges. Some faint features are discernible, possibly indicative of spiral arms or dust lanes, though the resolution makes this uncertain. The overall color appears to be somewhat redder, implying an older stellar population with ongoing star formation. There is no obvious sign of a major ongoing merger, but it is not possible to rule out some minor interaction or past merger event, and the general shape appears slightly disturbed.
