The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core is a bright, yellowish hue suggesting a population dominated by older stars.  There is a slight elongation to the shape, deviating subtly from a perfectly circular form.  No distinct spiral arm structures or significant dust lane features are readily apparent.  Faint, diffuse extensions surround the central region, possibly indicative of a stellar halo or the result of past minor interactions.  Overall, the galaxy appears relatively isolated and undisturbed, showing no strong signs of ongoing or recent major merger events.
