The galaxy presents as a slightly elongated, lenticular structure, appearing generally smooth with a subtle disk. There is a bright central bulge, potentially indicative of a supermassive black hole. The colour gradient shifts from yellow-white at the center, hinting at a population of older stars, to a blue-green hue in the outer regions, possibly suggesting areas of active star formation. The galaxy does not exhibit strong spiral arm structures or significant signs of ongoing major mergers. There is a slight asymmetry to the galaxy's halo but this is not indicative of any major disturbance to the galaxy. The galaxy is generally isolated, indicating that it has not undergone recent mergers or tidal disruption.
