The galaxy appears as a centrally concentrated object with a predominantly smooth morphology. It exhibits a bright core, suggesting a significant concentration of stars or potentially an active galactic nucleus. The overall shape appears largely rounded, showing minimal elongation or distortion. There is faint, diffuse light extending outwards from the core, but no distinct spiral arms or bar structures are discernible in this image. There appears to be a slight asymmetry in the light distribution, with a subtle extension of light towards the upper left. The color profile suggests a mix of stellar populations, though the overall color appears relatively uniform with a slight blue tint. There are no obvious signs of recent or ongoing major mergers, tidal tails, or strong gravitational disturbances.
