The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light profile. There's no visible spiral arm structure or prominent dust lanes. The color suggests a population of older stars, trending toward redder hues, implying a relatively low rate of ongoing star formation. The overall shape is moderately elliptical, not perfectly spherical, and exhibits no obvious signs of major mergers or significant tidal disturbances in its immediate vicinity, although minor interactions cannot be ruled out. The galaxy's core seems bright, possibly indicating the presence of a supermassive black hole or a dense stellar population.
