The galaxy presents as a moderately luminous, elongated structure. Its apparent shape is suggestive of a disk galaxy viewed at a highly inclined angle. There is a subtle color gradient present, with a central bulge exhibiting a yellowish hue, possibly indicating an older stellar population. Fainter, bluish hues are observed in the outer regions of the disk, suggesting the presence of younger, hotter stars and potential star forming regions, although distinct spiral arm structures are not clearly resolvable. Overall, the galaxy appears relatively undisturbed, without significant signs of ongoing mergers or tidal interactions.
