The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is moderately elongated, appearing more oblong than perfectly spherical. The central region exhibits a concentrated luminosity, suggesting a significant stellar population density. The color profile shifts from a warmer, reddish hue in the core to a cooler, bluish tinge in the outer regions, potentially indicating differing stellar populations or dust distribution. There is little evidence of distinct spiral arms or prominent dust lanes, supporting its classification as a spheroid-dominated system. Slight asymmetries in the outer halo may suggest minor gravitational interactions or past mergers, but these are not strongly pronounced. The galaxy appears to be relatively isolated in this field, with no immediate signs of major ongoing mergers or tidal disruptions.
