The galaxy appears to be a relatively smooth, elliptical type. Its light profile exhibits a strong central concentration, indicative of a substantial bulge component. There is no visible evidence of spiral arms or a prominent disk structure. The galaxy presents a uniformly diffuse, yellowish hue, suggestive of an older stellar population with minimal ongoing star formation. The morphology seems largely undisturbed, showing no signs of major mergers or tidal interactions. The overall round shape is highly suggestive of an E0-E3 classification on the Hubble sequence. The size is moderate compared to other galaxies, with a clearly defined edge to the extended halo. 
