The galaxy presents an elliptical morphology, exhibiting a high degree of central concentration. It appears relatively smooth in texture, with a gradual decrease in luminosity from the core outwards. No distinct spiral arms or bar structures are readily apparent. The color profile suggests a population dominated by older stars, with a subtle shift towards redder hues in the outer regions. There is no strong evidence of active star formation, indicating that the galaxy is likely quiescent or undergoing a period of suppressed star formation activity. There may be a very small, subtle asymmetry or tidal feature, but overall this galaxy is relatively undisturbed. The galaxy exhibits a luminosity consistent with that of a small, older galaxy.
