The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually fades into its outer regions, with no apparent spiral arm structures. The color profile suggests an older stellar population, as indicated by its redder hue in the image. The overall shape is neither perfectly spherical nor highly elongated, appearing to be more of an intermediate elliptical form. There is no distinct evidence of ongoing major merger activity or significant tidal disturbances. The galaxy appears relatively isolated, with no close companions that would suggest strong gravitational interactions, although subtle irregularities in the isophotes suggest minor disturbances could be present.
