The galaxy presents a relatively smooth morphology, with a centrally concentrated luminosity profile. It appears elliptical or possibly lenticular. The object exhibits a subtle color gradient; the central region appears slightly redder than the outer parts, suggesting a population of older stars in the core. The overall color indices indicate a moderately evolved stellar population, with minimal evidence of ongoing active star formation. There appears to be some minor tidal disturbance suggesting past or ongoing interactions with another galaxy, however, it does not appear to be a major merger. The galaxy exhibits intermediate roundness, leaning towards an elliptical shape.
