The galaxy presents as a luminous elliptical form, elongated along its major axis. Its color profile indicates a relatively mature stellar population, with a predominantly redder hue emanating from the central bulge. The galaxy exhibits a smooth, diffuse appearance, with no readily discernible spiral arm structures. The light distribution appears centrally concentrated, gradually decreasing in intensity towards the outer regions of the galaxy. There may be a slight warp or minor disturbance in the galaxy's morphology, but it is not significantly disrupted.
