The galaxy presents as a generally smooth, elliptical-like structure with a concentrated, bright central bulge. The light distribution appears fairly uniform, lacking any prominent spiral arm features or dust lanes. The color profile indicates a redder hue, particularly concentrated in the core, suggesting a population of older stars. The outer regions exhibit a slightly bluer tint, implying the presence of some younger stellar populations, though less dominant. There's no obvious evidence of strong ongoing star formation, nor are there any clear signs of tidal disturbances or interactions with other galaxies. The shape is close to circular, with only a slight deviation from perfect roundness.
