The galaxy presents a largely smooth and centralized morphology. It is a relatively compact system, exhibiting a near-circular profile. A bright, concentrated central bulge dominates the galaxy's structure, fading outwards into a less distinct halo or disk component. The color profile suggests a mix of stellar populations, with a warmer, yellowish hue at the core, likely indicative of older stars, surrounded by a bluer region that suggests ongoing, albeit modest, star formation. There is no clear indication of spiral arms, bars, or other prominent features within the disk. No signs of tidal disturbances or interactions are evident, indicating that the galaxy is likely in a relatively quiescent state, unperturbed by recent mergers. 
