The galaxy presents as a centrally concentrated object. Its overall morphology appears relatively smooth, lacking any distinct spiral arms or a prominent bar structure. The galaxy exhibits a slightly elongated shape, with an ellipticity that is not extreme. There may be a very slight suggestion of a faint disk structure, though not clearly defined. The galaxy's color suggests a mixed stellar population, without a strong dominance of either young blue stars or older red stars. There is no obvious evidence of ongoing major merger activity or significant tidal disturbances in the immediate vicinity of the galaxy.
