The galaxy presents as a single, relatively smooth and concentrated light source. Its overall shape appears approximately circular, lacking any obvious spiral arm structures or bar features. The central region exhibits a higher surface brightness, indicating a concentrated nucleus or bulge component. A slight color gradient is visible, with the core appearing more yellowish-white, transitioning to a slightly redder hue in the outer regions. This color profile could suggest an older stellar population dominating the central region, with a potentially younger, bluer population contributing to the outer regions. There is no indication of any major mergers or tidal disturbances in this image, although minor interactions cannot be ruled out at this resolution. The apparent smoothness suggests a lack of significant dust lanes or active star formation regions easily discernible from this perspective. 
