The galaxy presents as a relatively compact object, exhibiting a predominantly smooth morphology. Its shape is generally elliptical, with the ratio of the major to minor axis appearing close to one, indicative of a near circular projection on the sky. No distinct spiral arm structures or a prominent galactic bar are discernible. There is a slight indication of disturbed morphology suggesting potentially minor gravitational interaction with another object or past merger event. The galaxy exhibits a color gradient, with a core showing a slightly redder hue compared to its outer regions. The overall color suggests a population dominated by older stars, with moderate star formation activity. The galaxy appears as an isolated object, not obviously embedded within a dense cluster environment.
