The galaxy exhibits a generally elliptical morphology. It displays a smooth, concentrated central bulge that dominates the overall light profile. The outer regions of the galaxy fade gradually away from the center, showing a less defined disk structure. There is some asymmetry present, with the upper right portion of the galaxy appearing slightly disturbed or elongated compared to the rest of the disk. The core is quite bright, with a Sersic index value indicating a significant amount of light concentrated toward the center. Colors are typical of an older stellar population, with a redder hue indicating a lower rate of star formation. The presence of a low star formation rate is also consistent with the smooth morphology and lack of prominent spiral arms.
