The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light distribution. The core region is characterized by a bright, yellowish-orange hue, suggesting a population of older stars. Moving outwards from the center, the color gradually shifts towards a less saturated, darker red-orange. There is no discernible spiral arm structure or dust lane obscuration within the observable morphology. The galaxy's overall shape is elongated, with the major axis significantly longer than the minor axis, appearing cigar shaped. No evidence of tidal tails or major mergers is apparent, although there is a slight unevenness in the outer halo region on one side, possibly indicating a minor interaction or disturbance. The galaxy possesses a diffuse halo.
