The object appears to be a relatively distant galaxy, exhibiting an elongated, cigar-shaped morphology. The central region displays a noticeable concentration of light, suggesting a prominent galactic bulge. The color gradient shifts from a yellowish hue in the core to slightly bluer tones towards the outer edges. There is no apparent spiral structure, which suggests the galaxy is lenticular or elliptical. The lack of significant irregularities or tidal features indicates that the galaxy is relatively undisturbed and not currently undergoing a major merging event. Based on the color profile, the galaxy likely has a substantial population of older stars within the central bulge, while star formation may be occurring at a moderate rate in the outer regions.
