The galaxy presents a predominantly smooth morphology, exhibiting a slight elongation. The radial color gradient suggests a relatively older stellar population concentrated in the central bulge, characterized by a yellowish hue. The outer regions show a subtle transition toward bluer tones, possibly indicating the presence of younger stars and ongoing star formation at a lower rate. Faint, diffuse features can be observed in the outer disk, hinting at minor gravitational interactions or internal dynamics affecting its structure, but the overall structure appears relatively undisturbed, with no signs of significant tidal tails or strong distortions. The galaxy's light profile is moderately concentrated, suggestive of an intermediate-mass system.
