The galaxy presents as a centrally concentrated, smooth elliptical with an apparent round morphology. The light distribution appears relatively uniform, lacking any distinct spiral arms or bar structures. The color index suggests a population of older stars, with a higher concentration of redder wavelengths. There is no indication of ongoing major star formation activity or significant dust lanes. The galaxy exhibits a degree of central concentration, however, the galaxy appears homogenous. There is no apparent distortion in the galaxy's overall shape, leading to the conclusion that there has been no recent major merging activity. There is a relatively low likelihood of the galaxy being involved in a merger.
