The galaxy presents as a luminous, elliptical object, exhibiting a generally smooth morphology. There is little evidence of significant star formation activity based on the lack of strong blue color, suggesting an older stellar population. The light is concentrated towards the center, indicating the presence of a prominent galactic nucleus. The color gradient transitions from redder hues in the core to slightly bluer tones in the outer regions, which may indicate some population of younger stars at the outer edges. The galaxy appears largely undisturbed, with no major signs of recent mergers or tidal interactions. There is some evidence of a subtle disk-like structure, however, the dominant feature is smooth and spheroidal. It appears to be in a relatively quiescent state, with low current star formation rate.
