The galaxy presents as a relatively smooth, elliptical structure. The light profile appears centrally concentrated, exhibiting a bright core that gradually fades outwards. The galaxy appears to be reasonably round. No prominent spiral arms or distinct dust lanes are visible. There is some slight blueness, particularly towards the galaxy's center, suggestive of ongoing star formation. The overall color is indicative of a galaxy comprised of an older stellar population, however, the slight blueness indicates that there is likely some current star formation. There is no indication of any major mergers or disturbances in the galaxy’s morphology, however there is a slight irregularity to the galaxy which could suggest a minor merger in the past, or currently ongoing.
