The galaxy presents a smooth, elliptical morphology. Its core exhibits a concentrated, luminous intensity, appearing yellowish. The shape is somewhat elongated, approximating a cigar shape, although it primarily resides between perfectly round and significantly elongated. The galaxy exhibits a lack of discernible spiral arm structures or notable disk features within the resolution limits of this image. There are no strong indications of ongoing or recent major mergers or significant tidal disturbances. Any minor disturbances are ambiguous within the image resolution. The color profile suggests an older stellar population dominated by redder wavelengths, with a lack of prominent blue star-forming regions, consistent with a low star formation rate. The galaxy is estimated to have a substantial mass.
