The galaxy appears to be an interacting system, possibly in the early stages of a merger. One component exhibits a relatively smooth, elliptical morphology with a concentrated central bulge. Its color suggests an older stellar population, potentially dominated by redder giant stars. The second component appears bluer in color, possibly indicating more recent or ongoing star formation. This galaxy's morphology is less defined, appearing more disturbed or irregular. There are faint hints of tidal features or distorted arms suggesting gravitational interaction between the two components. The overall system has an intermediate luminosity, with evidence of moderate star formation activity relative to its mass.
