The galaxy presents as a concentrated, luminous object, with a smooth, elliptical morphology. The central bulge appears as a dominant, bright region, gradually fading outward into a less defined halo. There's a noticeable lack of distinct spiral arm structures or prominent dust lanes. The color profile appears to be relatively uniform across the galaxy, suggestive of an older stellar population. No obvious signs of ongoing major mergers or tidal disturbances are apparent. Faint indications of minor disturbances might be present, but they are indistinct. The galaxy is observed to have a slightly elongated shape, deviating from a perfectly circular form.