This galaxy appears to be a relatively small, elongated, and isolated system. Its light profile is dominated by a smooth, centrally concentrated bulge. The galaxy exhibits an orange-yellow hue, suggesting a population of older stars. The shape of the galaxy is indicative of an elliptical galaxy, likely of type E4-E6, though a lenticular classification (S0) is not out of the question due to its slight disk-like appearance. There is little to no visible dust or gas, and no prominent spiral arms are apparent. There does not appear to be any current merger activity or obvious signs of tidal disturbances, though the presence of minor perturbations is not entirely excluded. The galaxy appears to be quiescent, with a low rate of star formation.
