This galaxy presents a relatively smooth and featureless appearance. It exhibits an elliptical morphology, appearing mostly round but possibly slightly elongated. The galaxy displays a color gradient, with a yellowish core that suggests an older stellar population and a less active star formation rate in the central region. There is little evidence of spiral arms or significant dust lanes. The galaxy appears to be isolated, with no obvious signs of interaction or recent merger activity. Some indications suggest the galaxy may have undergone some minor disturbance in its past, or possibly be in the early stages of a minor merger event, but further examination is needed to confirm. The relatively homogenous appearance is indicative of a high degree of symmetry and suggests an evolved dynamical state.
