The galaxy presents as a central, somewhat concentrated object with a smooth, elliptical morphology. It appears to have a centrally concentrated bulge, lacking prominent spiral arms or a well-defined disk structure. The galaxy exhibits a relatively uniform color profile, dominated by redder hues throughout, suggesting an older stellar population. The absence of significant blue regions indicates a low rate of ongoing star formation. There is evidence of some minor disturbances or irregularities in the galaxy's shape, possibly due to a past interaction or minor merger event. No prominent dust lanes or tidal tails are apparent in the image. Overall, the galaxy appears to be a relatively massive, evolved system.
