The galaxy presents as a concentrated, centrally luminous object with a generally smooth appearance. The overall shape is observed to be roughly elliptical. There is a slight indication of some minor asymmetry, but no distinct spiral arms or bar structures are discernible in the available imagery. The galaxy emits light across the visible spectrum, with a peak emission in the redder wavelengths, suggesting a population of older stars and a relative lack of significant ongoing star formation. The color profile indicates a significant fraction of the stellar population may be evolved, implying a more quiescent star formation history. The morphological classification points towards the galaxy being of an early-type, potentially an elliptical galaxy or a lenticular galaxy with a dominant bulge.
