The galaxy presents a generally smooth morphology. The primary light distribution appears concentrated towards the central region, exhibiting a somewhat elliptical shape, although the roundness is fairly high. Some subtle irregularities are observed in the outer regions, hinting at possible tidal interactions or minor disturbances, but these are not prominent. The color profile suggests a population dominated by older stars, with a redder overall hue. There is no clear evidence of prominent spiral arms or a well-defined disk structure. The galaxy appears to be relatively isolated, showing no obvious signs of a major ongoing merger. The overall structure suggests a system that is relatively evolved and stable.
