The galaxy presents as a smooth, elongated structure, suggestive of an elliptical or lenticular morphology. The central region exhibits a high surface brightness, with the light gradually diminishing towards the outer edges. No distinct spiral arms or dust lanes are discernible. The color appears generally blue, perhaps indicating a population of younger, hotter stars, though this is contrasted by the relatively smooth and featureless morphology typically associated with older stellar populations. There appears to be little to no evidence of active merging or major disturbances, as the galaxy presents a fairly regular structure. The elongation suggests that this is not a perfectly spherical system, but is perhaps viewed at a slight angle.