The galaxy presents as a single, largely featureless object. It appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated luminosity profile. There is an absence of spiral arms, dust lanes, or other distinct morphological features typically associated with disk galaxies. The light distribution exhibits a high degree of radial symmetry, with a slight elongation along one axis. The core is luminous, grading outwards into a slightly fainter halo. In terms of color, the galaxy displays a yellowish-white hue in the core, suggestive of an older stellar population dominating the light output. The outer regions exhibit a faint reddish tint. There is no indication of significant ongoing star formation activity based on color indices, and no major merger events appear to have taken place recently, as the galaxy displays a well-defined, undisturbed morphology.
