The galaxy presents as a system comprised of two distinct components, suggestive of an ongoing or recent merger event. The primary component exhibits a relatively smooth, elliptical morphology, with a concentrated, luminous core region. The color profile appears to be broadly consistent with an older stellar population, characterized by a yellowish hue. A secondary, smaller component is visible nearby. There is some visual suggestion of tidal disturbances or disrupted morphology, particularly around the brighter object. The galaxy appears to be in a relatively quiescent state of star formation.
