The galaxy presents an overall elliptical morphology with a high degree of central concentration. Its smooth light profile suggests a lack of significant spiral arm structure. The core region exhibits a yellowish-white hue, indicative of an older stellar population likely dominated by red giants. Moving outwards from the core, the color transitions towards a slightly bluer shade, suggesting the presence of a younger stellar population, but still significantly subdued. No significant dust lanes or prominent star-forming regions are visible, suggesting a relatively low star formation rate. The galaxy appears generally undisturbed, without any obvious signs of recent major merger events or tidal interactions. It appears relatively isolated within its environment. The isophotes are generally elliptical and concentric, indicating a stable and relaxed system. The estimated size suggests it is a moderately sized galaxy.
