The galaxy presents a generally smooth, elliptical morphology. It appears quite concentrated, with a bright central region that gradually diffuses outwards. The core exhibits a yellowish hue, possibly indicating a population of older stars. There is faint bluer light at the periphery which may indicate some star forming regions, but the overall rate of star formation appears to be relatively low. No distinct spiral arm structures are visible; however, a hint of minor disturbance, likely due to past interactions with smaller objects or uneven accretion, is visible in the asymmetry of the fainter surrounding halo. The object appears fairly isolated, with no major signs of active merging or significant tidal distortions from gravitational interactions with other galaxies. The galaxy's round shape and central concentration suggests it is a mature system which has undergone significant dynamical evolution.
