The galaxy exhibits a primarily smooth morphology, appearing largely elliptical in shape, although subtle features or a disk component cannot be entirely ruled out. The central region displays a high concentration of light, suggestive of a prominent galactic nucleus or bulge. The light profile becomes more diffuse towards the outer regions of the galaxy.  Color gradients are subtle, with the central bulge tending towards a slightly yellow hue, which could indicate an older stellar population. The overall structure gives the impression of a relatively relaxed system, showing no strong signs of a major recent merger or significant tidal disruption. There may be some minimal disturbance. The galaxy's overall apparent size is modest, suggesting it could be a dwarf galaxy or a more distant object.
