The galaxy appears as a smooth, elongated structure, potentially an elliptical or lenticular galaxy viewed at an angle. Its central region exhibits a higher surface brightness, indicating a concentrated core. The light distribution fades gradually towards the outer edges, forming a diffuse halo. There is a slight color gradient from the center outwards, suggesting a change in stellar populations. The overall appearance lacks any distinct spiral arms or irregular features, supporting a classification as a relatively undisturbed system. The shape appears to be more cigar shaped than round. No evidence of significant dust lanes or recent merger activity is apparent in this image.