The observed galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a higher surface brightness and a yellowish-white coloration, suggesting an older stellar population concentrated towards the core. Moving outward from the center, the galaxy gradually fades in brightness with hints of a bluer color, indicating the presence of a younger, more actively star-forming population. Though somewhat obscured by the distance and likely dust, there is a subtle disc-like structure surrounding the bulge. Overall, the galaxy appears relatively smooth and undisturbed, with no readily apparent major tidal features or signs of significant merger activity.
