The galaxy presents as a generally smooth, elliptical object. Its morphology is somewhat elongated, appearing more cigar-shaped than perfectly round. The central region exhibits a higher concentration of luminosity, gradually decreasing outwards. There is a noticeable color gradient within the galaxy. The central region appears yellower and redder compared to the outer regions, which exhibit a bluer hue. No significant dust lanes or prominent spiral arm structures are discernible. The galaxy exhibits a general lack of significant morphological disturbances or indications of major ongoing merging events. The galaxy is observed to have a moderately high redshift, and has an estimated size of approximately 6 kpc. This observation indicates that the galaxy is relatively massive and possesses a moderate rate of star formation.
