This galaxy exhibits a complex morphology. The central region appears to be dominated by a bright, concentrated bulge, showing a gradient from yellow-white in the core to reddish hues towards its periphery. This could indicate a population of older stars in the outer bulge regions.

Extending laterally from the central bulge are two distinct, irregular structures. These appear somewhat fragmented and exhibit redder colors than the bulge, potentially signaling the presence of dust lanes or regions of active star formation obscured by dust. There is a faint bluish emission extending out on one side, which might be recent star formation. Overall, the galaxy does not present a smooth, well-defined structure; it is more disturbed. This galaxy could be undergoing tidal disruption or have experienced a recent merger.
