The galaxy presents a relatively smooth, elliptical morphology. Its central bulge exhibits a high degree of concentration, appearing nearly spherical and possessing a yellow-white hue, suggestive of an older stellar population. Moving outward from the core, the light fades gradually, forming an extended halo. The galaxy is not perfectly spherical, showing a slight elongation or cigar shape. There is no evidence of spiral arm structure or significant dust lanes. The overall color profile indicates that the galaxy is dominated by older stars, suggesting a relatively low star formation rate at present. Faint tidal features or minor disturbances may be present, though the image resolution limits conclusive identification.
