The galaxy appears to be a relatively smooth, centrally concentrated object. The core exhibits a yellowish hue, suggesting a population of older stars. Moving outward from the core, the galaxy's light fades, and a hint of bluer color is observed in the outer regions. The shape is roughly round, with minimal evidence of spiral arms or a well-defined disk structure. There is a slight irregularity in the outer edges. Overall, the galaxy appears to be an elliptical galaxy with a modest amount of recent or ongoing star formation occurring in its outer regions. It does not appear to be undergoing a major merger or experiencing strong tidal disturbances.
