The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution is concentrated towards the center, indicating a higher density of stars in the galactic nucleus. There is a noticeable decrease in luminosity moving outward from the core with an elliptical shape. The color profile appears slightly redder than typical spiral galaxies, suggesting a population of older stars and a lower rate of active star formation, consistent with early-type galaxies. There is a possible minor disturbance to the galaxy. The galaxy does appear relatively isolated and does not appear to be undergoing any major interactions.
