The galaxy appears as a slightly elongated elliptical structure, with an estimated effective radius of approximately 2.4 kpc. The central region exhibits a bright, concentrated core that gradually fades into the outer regions. The overall light distribution is smooth, suggesting a lack of significant spiral arms or prominent star-forming regions. The ellipticity is moderate, indicating a relatively flattened shape. There is a slight color gradient, with the core appearing yellower, potentially indicating an older stellar population. There is no significant evidence of tidal tails or major disturbances, which suggests that this galaxy is not undergoing a major merger or interaction. There is some evidence of possible dust lanes.
