The galaxy presents a generally smooth, elliptical morphology. Its light distribution appears fairly concentrated, with a gradual falloff from the core. No distinct spiral arms or bar structures are discernible. The color profile suggests a population of older stars, with a higher proportion of redder wavelengths. This indicates a lower rate of ongoing star formation within the galaxy. There is no evidence of any major tidal disturbances, merging events, or significant dust lanes obscuring the galactic nucleus. Overall, the galaxy appears to be relatively undisturbed and quiescent.
