The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge that appears yellowish, suggesting an older stellar population dominating its core. The galaxy's overall shape is elongated, trending towards a cigar-like form. A faint, diffuse halo surrounds the central region, exhibiting a bluer hue, possibly indicating the presence of younger stars or ongoing star formation at a relatively low rate in the outer regions. There is no evidence of significant spiral arm structure or major disturbances indicative of recent major mergers. Minor disturbances in the outer halo cannot be ruled out.
