The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region displays a yellowish hue, suggestive of an older stellar population. Moving outward, the color gradient shifts towards redder tones. The overall shape is elongated. There is very little evidence of spiral arm structure or prominent dust lanes. Faint tidal features or minor disturbances are not detectable in this image. The galaxy appears relatively isolated, with no obvious signs of ongoing or recent major mergers. 
