The galaxy presents as a concentrated central bulge of moderate brightness, gradually fading into a more diffuse halo. There are faint, extended features, possibly indicative of a disk-like structure or tidal tails. Based on the slight irregularity in its shape, it's possible it could be involved in a minor gravitational interaction, such as a merger or a close encounter, which is causing the faint distortions around the core. There is little, if any, evidence of spiral arm structure, but given the overall fuzziness of the galaxy, it's hard to make any definite conclusions about the disk. The color appears predominantly red, suggesting an older stellar population.
