This galaxy presents an elliptical morphology, appearing moderately elongated with a somewhat cigar-shaped profile. Its overall structure is relatively smooth, lacking prominent spiral arms or other distinct features. The color distribution reveals a central region dominated by redder hues, potentially indicative of an older stellar population. Moving outwards, the galaxy exhibits a gradual transition towards bluer tones, which may suggest the presence of younger stars or ongoing star formation activity. The galaxy appears largely undisturbed, showing no significant signs of major mergers or tidal disruptions, though subtle irregularities are present, hinting at possible minor disturbances or interactions. Overall, this galaxy seems to be a moderately massive system with a combination of old and potentially more recent stellar populations, exhibiting a relatively smooth and somewhat elongated structure.
