This galaxy presents a relatively smooth morphology, with a moderately elongated, cigar-shaped appearance. A distinct central bulge is visible, appearing brighter and more concentrated than the surrounding regions. The disk component, if present, is not clearly resolved into spiral arms. The color profile suggests a redder core region, potentially indicative of an older stellar population or dust obscuration. Moving outward from the core, the galaxy exhibits a slightly bluer hue, potentially reflecting younger stars within the disk. There is no obvious evidence of strong tidal features, merging activity, or significant star formation regions based on its overall smooth appearance. Its light distribution appears to be fairly symmetric about the center.