The galaxy presents a generally elliptical morphology, appearing quite smooth with a high degree of central concentration. The light distribution graduates outwards from a bright, almost unresolved core. There's a subtle color gradient evident, with the core exhibiting a yellowish hue, suggesting an older stellar population. Moving outwards from the central region, the galaxy appears slightly redder in its periphery, possibly indicating a larger proportion of older, redder stars or dust obscuration. The isophotes, based on visual inspection, seem relatively regular, with no obvious signs of strong tidal disturbances or ongoing major mergers. There might be some very subtle irregularities in the outer regions, but these are not prominent. The overall impression is that of a relatively undisturbed, evolved galaxy.
