The galaxy presents as a relatively small, elliptical object with a smooth, concentrated luminosity profile. Its overall shape is elongated, appearing cigar-shaped. There is an absence of prominent spiral arms or significant substructure within the galactic disk. The color is generally redder, suggesting a population of older stars and a dearth of ongoing, high-mass star formation. There may be an extremely faint and indistinct ring structure in the central region. The galaxy does not appear to be undergoing any major merger events or significant tidal disturbances based on its morphology.
