The galaxy presents an overall elliptical morphology, appearing largely smooth and featureless at this resolution. The light distribution indicates a concentration of older stars towards the center, as evidenced by the yellowish hue of the core. Progressing outwards, the galaxy gradually transitions to bluer tones, suggesting a population of younger, hotter stars in the outer regions and possibly ongoing, or recent, star formation. There is a slight asymmetry observed in the outer regions, which could potentially be indicative of a minor interaction or disturbance with a smaller companion. The shape is mostly round, not particularly elongated or cigar-shaped. There is no evidence of a distinct spiral structure or a prominent disk. Overall, the galaxy appears to be relatively quiescent with a moderate rate of star formation.
