The galaxy presents as a somewhat diffuse, centrally concentrated system, appearing largely smooth in overall structure. It exhibits a subtle elongation, deviating slightly from a perfectly circular form, leaning more toward an elliptical shape. The galaxy's core region demonstrates a higher luminosity, suggesting a dense concentration of stars. There appears to be a faint, extended halo surrounding the central body, gradually fading into the background sky. There is some evidence of minor tidal disturbance in the form of a slight asymmetry, potentially indicative of a past or ongoing interaction with another galaxy. Star formation appears to be present but subdued. The light is dominated by older stellar populations, which corresponds to lower levels of star formation. This galaxy appears relatively massive.
