The galaxy presents as a moderately luminous, compact object with an apparent spheroid morphology. It appears centrally concentrated. The color profile exhibits a yellow-orange hue, suggesting a population of older stars, and relatively little ongoing star formation. There is some slight color variation within the galaxy, indicating possible substructure or regions of varying stellar populations, however the resolution does not allow for a clear distinction. There is some apparent merging, perhaps more than one event, as well as possible tidal disturbances. Overall, the galaxy appears to be in the process of merging and is on the high side of having little to no star formation.