The galaxy presents as a generally smooth, elliptical morphology. The central bulge is a bright, concentrated region exhibiting a yellowish hue, suggesting an older stellar population. The isophotes appear mostly regular, with a fairly circular form. The outer regions of the galaxy fade gradually, displaying a slightly redder color than the core. This color gradient likely reflects differences in stellar age and metallicity distributions. There's a faint indication of a possible tidal feature or minor disturbance in the galaxy's outer halo, perhaps indicating a past minor merger event. Star formation appears to be suppressed within the galaxy.
