The galaxy presents a generally smooth appearance, with a concentrated central region exhibiting a yellowish hue. This central component likely contains a high density of older stars. The surrounding areas display a fainter, more diffuse structure with subtle hints of bluer coloration. These bluer regions suggest the presence of younger stellar populations and ongoing star formation, albeit at a low rate. There is a slight elongation to the galaxy's shape, deviating from a perfectly circular morphology. A minor asymmetry or disturbance is visible on one side of the galaxy, potentially indicating a past or ongoing interaction with a smaller companion or tidal effects. The overall structure appears relatively undisturbed, lacking prominent spiral arms or significant morphological complexities.
