The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is generally round, lacking any obvious spiral arms or a distinct disk structure. The color profile suggests a dominant population of older stars, evidenced by the yellowish hue, particularly in the central bulge. The outer regions appear slightly bluer, possibly indicating a minor presence of younger stellar populations. There is no strong evidence of active star formation or significant dust lanes obscuring the light. The overall morphology indicates that this is likely an elliptical galaxy, or potentially a lenticular galaxy with a very faint disk. No major mergers or disturbances are apparent in its structure, suggesting it has evolved relatively undisturbed over a significant period.
