The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated light distribution. The core exhibits a bright, yellowish hue, which is indicative of an older stellar population. A faint, extended halo surrounds the core, with light gradually fading outwards. There is little to no evidence of spiral arms or prominent dust lanes. The galaxy's shape deviates slightly from a perfect circle, appearing somewhat elongated. No major signs of recent merger activity or significant disturbances in its overall structure are observed, although there could be minor disturbances. The colour suggests moderate activity, but it is clear the galaxy is mostly comprised of older stars.
