The galaxy presents a centrally concentrated, generally smooth morphology. The light distribution is relatively uniform, lacking any prominent spiral arm structures or a well-defined bulge component. The shape is more in between than round or cigar shaped.

Color gradients suggest a relatively old stellar population, although some pockets of younger, bluer stars are present toward the center. These regions may indicate recent or ongoing star formation activity, although the overall rate appears to be low.

There is no obvious visual evidence of significant tidal features or interactions with nearby galaxies, suggesting that it has not undergone any major mergers recently.
