The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that is yellowish-orange in color, indicative of an older stellar population. There is a slight elongation to the galaxy's overall shape, appearing more lenticular than perfectly spherical. The outer regions of the galaxy appear fainter and slightly bluer, suggesting the presence of a younger stellar population, although this is not strongly pronounced. There is no visible dust lane or prominent spiral arm structure. Faint signs of disturbance in the halo may indicate a past minor merger event. The galaxy appears to be at an intermediate redshift. Overall, this galaxy appears to be an early-type galaxy with signs of modest star formation.
