The galaxy presents as a slightly elongated, lenticular-like object. It exhibits a subtle disk-like morphology, although its features appear generally smooth rather than showing distinct spiral arms or bar structures. The light distribution suggests a central bulge. The galaxy exhibits a subtle colour gradient, appearing slightly bluer towards the outer regions, which may indicate the presence of some ongoing star formation in the disk, though overall, the galaxy's color suggests an older stellar population. There is no indication of any major mergers or significant tidal disturbances from the images.
