The galaxy presents as a relatively compact, elliptical or lenticular-like structure. Its light profile is smooth and centrally concentrated, with a discernible core. No prominent spiral arms or bar features are visible, supporting the assessment of a smooth morphology. The light distribution is predominantly yellowish, suggesting a stellar population dominated by older stars. A slight elongation is present. There is no evidence of a major merger. Star formation appears subdued. The galaxy demonstrates significant mass.
