The galaxy presents a predominantly smooth morphology, indicative of a relatively old stellar population. It appears largely spheroidal, with a high degree of central concentration. There is a subtle color gradient observable, transitioning from a yellowish hue in the core to a slightly bluer color in the outer regions, suggesting a radial variation in stellar populations or dust content. No obvious spiral arm structures or prominent dust lanes are visible. The overall form suggests the galaxy is elliptical, or possibly an early-type spiral with a dominant bulge and tightly wound arms not resolvable at this scale. The moderate redshift suggests this is a reasonably distant object. There are subtle signs of a possible minor interaction, but overall the galaxy appears relatively undisturbed.
