The galaxy presents as a generally smooth object, with a concentrated central region and a diffuse halo. The light distribution appears axisymmetric and highly rounded. There are no discernible spiral arms or a bar structure; the galaxy seems to be an elliptical galaxy. Color gradients within the galaxy are subtle, suggesting a relatively homogeneous stellar population. No strong tidal features or indications of a major merger event are evident; however, there is a slight irregularity in the halo that may indicate a minor disturbance or recent accretion event. The galaxy does not show evidence of intense ongoing star formation, appearing relatively quiescent.
