The galaxy presents as an elliptical type with a smooth, centrally concentrated light profile. There is a distinct yellowish hue to the central bulge region, suggesting an older stellar population. The outer regions of the galaxy exhibit a gradual decrease in luminosity and shift towards slightly bluer colors. The overall shape is nearly circular, exhibiting minimal elongation. No prominent spiral arms, bars, or dust lanes are discernible. There are some possible faint features, which may be areas of ongoing star formation. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or mergers with other galaxies.
