The galaxy presents as an elongated, disk-shaped structure, likely a spiral or lenticular galaxy viewed at a high inclination. Its central region exhibits a concentrated, bright, yellowish-white luminosity, suggesting a substantial population of older stars. The disk appears relatively smooth, with only subtle variations in color and brightness and no readily apparent spiral arm structure. The galaxy appears to be isolated. Overall, the galaxy exhibits characteristics of an evolved system with a moderate stellar mass and low ongoing star formation activity.