The galaxy exhibits a predominantly smooth morphology, suggestive of an elliptical or lenticular type. There is little evidence of spiral arms or significant dust lanes. The central region displays a bright, concentrated luminosity, indicative of a dense stellar population and potentially an active galactic nucleus. The color profile demonstrates a redder hue in the core, which could indicate an older stellar population, while the outer regions show a bluer tint. The overall shape appears close to round. There is minimal, but non-zero, potential that a minor disturbance might be affecting the overall structure. It seems like this galaxy is experiencing a moderate level of star formation.
