The galaxy presents as a relatively smooth, elliptical-like structure with a dominant, bright central bulge. The light distribution appears concentrated towards the center, with a gradual decline in luminosity towards the outer regions. There is little evidence of prominent spiral arms or distinct features indicative of active star formation within the observable bands. The overall morphology suggests a mature system, potentially dominated by an older stellar population. There is a very slight hint of disk, but the overall shape does not deviate strongly from elliptical. No signs of major tidal disturbances or ongoing mergers are apparent, although there is a subtle asymmetry in the outer regions. The galaxy's color is yellowish, indicating a lack of blue light associated with young, hot stars, and a slight redshift.
