The galaxy presents as a relatively smooth, centrally concentrated object with a discernible spheroidal shape. There is a noticeable color gradient, transitioning from a yellowish-white core to a slightly bluer outer region. No distinct spiral arms or bar structures are apparent. The overall morphology suggests a possible elliptical galaxy, or potentially a spiral galaxy with a dominant bulge and tightly wound arms that are difficult to resolve at this resolution. There is no evidence of strong tidal disturbances or ongoing major mergers; however, minor irregularities in the outer envelope cannot be ruled out based on this image alone. The moderate blue color in the outer regions could indicate ongoing star formation, but this cannot be confirmed without spectroscopic data. The galaxy appears to be isolated, with no immediately interacting companions visible.
