The galaxy presents as a relatively smooth, disk-shaped structure. A bright, concentrated central bulge dominates the visual appearance. Extending outwards from the bulge is a disk component that appears to be only subtly featured, showing little evidence of strong spiral arms or other distinct structures. The overall color suggests a population dominated by older stars and possibly lower rates of current star formation, yet there seems to be a hint of blue, potentially indicating some younger stellar populations. The ellipticity indicates that the galaxy is likely seen at an angle, but it is closer to face-on than edge-on. There is little evidence of any major ongoing merger activity or significant tidal disturbances. The galaxy appears to be relatively isolated and undisturbed.
