The galaxy appears to be a lenticular or early-type spiral, exhibiting a generally smooth morphology. The central bulge is prominent and elongated, suggesting it is more cigar-shaped than perfectly round. There is a faint hint of a disk component, though any spiral arms are not well-defined or resolved. The light distribution within the galaxy appears relatively uniform, with no obvious signs of major disturbances or ongoing mergers, although a slight asymmetry cannot be ruled out. There is a nearby object that might possibly indicate a minor interaction, though it could also be a background or foreground source. The galaxy's overall color suggests an older stellar population with a relatively low rate of ongoing star formation.
