The observed galaxy exhibits a primarily smooth morphology, indicative of an elliptical or lenticular type. It possesses a distinctly elongated, cigar-like shape. The central region displays a concentrated luminosity, suggesting a substantial stellar population. A slight color gradient is visible, with the core appearing more yellow, possibly due to older stars and a lack of significant ongoing star formation, while the outer regions show hints of bluer hues. There is no strong evidence of spiral arm structures or significant dust lanes. No major disturbances or signs of recent mergers are apparent in the image, and there appears to be no tidal distortion to the overall galactic structure.
