The galaxy presents a largely smooth morphology. It appears elliptical with a high degree of roundness. The galaxy exhibits a concentrated central bulge that gradually fades into the outer regions. The color gradient suggests a population of older stars dominating the bulge, likely due to the yellowish hue observed. There are only faint hints of any spiral arm structures, indicating it is primarily composed of stars in a more spheroidal distribution. There are no obvious signs of a recent major merger event or significant tidal disturbances affecting its structure, although a very slight irregularity may be present. The estimated size indicates a moderate spatial extent. The blue-green color around the galaxy hints at some star formation.
