The galaxy presents as a moderately luminous, well-defined structure. It appears to be an elliptical or lenticular galaxy, demonstrating a primarily smooth morphology. The central bulge is bright, exhibiting a yellow-white hue, suggesting an older stellar population. There is a faint blue halo surrounding the bulge, possibly indicative of some ongoing, though minimal, star formation. The galaxy displays a slight elongation but is generally close to round. No distinct spiral arms or dust lanes are visible. There are hints of minor disturbances in its structure, potentially indicative of a past or ongoing minor interaction. The galaxy appears relatively isolated.
