The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The color profile suggests a predominantly older stellar population, characterized by a yellowish-orange hue concentrated in the center and diminishing outwards. There is little evidence of distinct spiral arm structures or prominent dust lanes. The galaxy appears somewhat elongated, with a moderate ellipticity. No significant tidal features or signs of recent major mergers are discernible, though a slight asymmetry could indicate a minor interaction or disturbance in its past. The overall morphology is consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy.
