The galaxy presents as a moderately bright, elliptical morphology with a smooth, diffuse light distribution. The core region exhibits a concentrated brightness, suggesting a spheroidal structure with a gradual decrease in luminosity towards the outer edges. The object has a notable color gradient, appearing bluer towards the central regions and shifting towards redder hues in the outskirts. The overall shape appears somewhat elongated, displaying a cigar-like structure. There is no obvious presence of spiral arms, dust lanes, or other distinct features typically associated with disk galaxies. The structure appears relatively undisturbed, with no strong visual evidence of recent major mergers or interactions. However, there is a hint of a slight disturbance in the distribution of light, suggesting a minor interaction or tidal feature. The object is compact, with a median radius of approximately 5 kiloparsecs. The galaxy displays an active star formation rate.