This galaxy exhibits a roughly elliptical morphology, appearing moderately elongated. The central bulge is prominent and displays a yellowish hue, suggesting an older stellar population and a lack of significant ongoing star formation in that region. Extending outwards from the core are fainter, disk-like structures, primarily bluish in color, which possibly indicates ongoing star formation. The edges of the disk are somewhat ill-defined, with no readily apparent spiral arms or bar features. Overall, the galaxy appears relatively undisturbed, although there is subtle irregularity in the outer regions of the disk, perhaps suggestive of a past minor interaction. There are no signs of a major merger. The estimated mass of the galaxy is considerable. The rate of star formation appears modest.
