The galaxy presents a generally smooth morphology, lacking prominent spiral arms or significant dust lanes. Its shape is elongated, appearing as a flattened spheroid, approaching a cigar-like form. The central region exhibits a concentrated brightness, suggesting a bulge component. The galaxy displays a color gradient, with the core appearing more yellow/white, potentially indicating an older stellar population, while the outer regions appear slightly bluer, perhaps hinting at ongoing or recent star formation. There is no visual evidence of major mergers or significant tidal disturbances. Faint, diffuse extensions might be present at the galaxy's edges, though this is difficult to ascertain due to image resolution.
