The galaxy presents a largely smooth and rounded morphology. There is an absence of clearly defined spiral arms or a prominent disk structure. The light distribution appears centrally concentrated, with a gradual decrease in brightness towards the outer regions. The color profile suggests an older stellar population, trending towards redder hues. There is no evidence of ongoing major merging activity or significant tidal disturbances, with the overall structure appearing relatively undisturbed. Star formation is present, but is at a low level.
