The galaxy presents as a centrally concentrated object with a generally smooth appearance. There is some suggestion of minor disturbances or irregularities in its structure, possibly indicative of past or ongoing interactions. The galaxy is moderately elliptical in shape, appearing neither perfectly round nor highly elongated. The light distribution is concentrated towards the core, with a gradual decrease in intensity outwards. While a disk-like structure is not obviously apparent, the presence of some slight irregularities cannot rule it out. The color suggests relatively old stellar populations, though the presence of some subtle color variation may suggest some on-going star formation. No obvious spiral arms or other major features are visible. There appears to be no major merger events evident. Overall, the galaxy appears to be a relatively isolated system, with some minor interactions.
