The galaxy appears to be a relatively smooth system, with a centrally concentrated, somewhat rounded morphology. The central region exhibits a brighter, slightly bluer hue, possibly indicating a region of ongoing star formation. The galaxy shows a more subtle disk structure. There is no apparent strong distortion or tidal features, suggesting that any recent mergers or interactions were minor, if present at all. The overall color profile suggests a galaxy with a mix of older stellar populations and some younger, bluer stars in the core.
