The galaxy presents a generally smooth morphology, exhibiting a concentrated central bulge. A faint, disklike structure is suggested by subtle color variations and a slight flattening. The galaxy's color profile suggests a dominant population of older stars, with redder hues concentrated in the central bulge and a bluer tint indicating some regions of ongoing star formation. There is some indication of minor gravitational disturbance. The central region exhibits high luminosity, implying a significant concentration of mass. Overall, the galaxy appears to be at an intermediate stage of evolution, transitioning from active star formation to a more quiescent state.
