The galaxy appears as an elongated, somewhat irregular structure. Its central region is dominated by a smooth, concentrated light distribution, which suggests the presence of a bulge, possibly containing an older stellar population. Extending from the bulge, a faint disk-like structure can be discerned, but it lacks sharply defined spiral arms. There is a slight asymmetry in the light distribution of the galaxy, hinting at possible tidal interactions. Towards one end of the disk, there is a subtle color change, appearing redder than the rest of the structure, which may indicate a region of dust obscuration or a population of older stars. Overall, the galaxy exhibits a blend of smooth and disturbed features.
