The galaxy appears to be elliptical in morphology, exhibiting a smooth, symmetrical light distribution. The core region shows a concentrated luminosity, suggesting a dense stellar population. The color profile transitions from a yellowish-white center to a more reddish hue in the outer regions, indicating older stellar populations are more prominent further from the center. There is little to no evidence of spiral arm structures or significant dust lanes. The galaxy appears to be relatively isolated with a round shape. The galaxy displays no signs of major disturbances or ongoing mergers. 
