The galaxy presents as a relatively smooth, elliptical structure. Its color gradient shifts from a yellowish core to a bluer outer halo, suggesting a declining star formation rate towards the nucleus. There is an overall smooth and elongated shape, without any prominent spiral arms or distinct features typically associated with disk galaxies. No significant distortions or tidal tails are readily apparent, indicating it has likely not undergone a major merger recently. The overall morphology suggests a system dominated by an older stellar population.
