The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decline in luminosity outward. The color profile suggests a generally older stellar population with a yellow-red hue. There is no apparent spiral arm structure or dust lane obscuration visible in this image. The galaxy appears fairly isolated, showing no immediate signs of tidal interactions or ongoing mergers with other galaxies. The overall morphology suggests a mature galaxy with a quiescent star formation rate.
