The galaxy presents as a moderately bright, relatively smooth object with a concentrated central region. The light distribution suggests a spheroidal morphology, potentially an elliptical galaxy, with a noticeable lack of distinct spiral arm structures. The galaxy appears to have a slight reddish hue, indicating a population of older stars. The galaxy exhibits a fairly uniform luminosity gradient from the core outwards, with no substantial features disrupting the smooth appearance. There may be a slight tidal disturbance on one side, but this is minimal and not a clear merger event. The roundness is not complete, with a slight elongation.
