The galaxy presents as a single, relatively compact object with a smooth morphology. There is no apparent spiral structure or bar. The galaxy's color profile suggests a slightly redder hue, indicative of an older stellar population or significant dust obscuration. It appears to be a single, somewhat rounded object with no obvious signs of tidal disruption or interaction with other galaxies. There is a very faint extension that may point to a minor disturbance. The overall light distribution is concentrated towards the center, suggesting a higher density of stars within the galactic core.
