The galaxy presents a generally smooth morphology with a centrally concentrated light profile. Its overall shape appears to be approximately elliptical but the minor axis seems slightly smaller than the major axis. The color profile is not uniform, displaying a distinct yellow hue in its core, suggesting an older stellar population and potentially less active star formation. A bluer color can be seen in the outskirts, indicative of the presence of younger, hotter stars, hinting at some ongoing or recent star formation activity in those regions. No prominent spiral arms or bar structures are discernible within the image's resolution limits. There's no evidence of strong tidal features, major disturbances, or ongoing mergers based on the structure present in the image. 
