The galaxy presents as an elliptical morphology, exhibiting a high degree of smoothness across its structure. It appears cigar shaped, with a color profile that indicates a slightly higher concentration of older stars. There is a general lack of distinct features such as spiral arms or prominent dust lanes. The overall light distribution suggests a centrally concentrated luminosity profile, typical of elliptical galaxies. There is no immediately obvious indication of any ongoing major merging activity or significant tidal disturbances affecting the galaxy's shape. However, some minor distortions are possible.