The galaxy exhibits a complex morphology, potentially indicative of an ongoing or recent merger event. The central region presents a relatively smooth, diffuse appearance, but there's evidence of disturbed structure. A pronounced, irregular extension or tidal tail-like feature emanates from the main body, suggesting gravitational interaction with another galaxy or significant internal dynamical processes. The overall color profile leans towards the red end of the spectrum, implying a population dominated by older stars, yet some bluer regions hint at more recent star formation activity. While a distinct spiral arm structure is not apparent, the presence of irregular features and color variations point to a galaxy undergoing significant evolutionary changes. Its shape could be classified as somewhere between round and elliptical. There appears to be a higher fraction of redder objects in the galaxy than bluer, and a medium mass with detectable star formation rates.
