The galaxy presents as an elliptical morphology with a high degree of central concentration. The core region exhibits a yellowish-white hue, suggestive of an older stellar population and relatively low ongoing star formation. Moving outward from the core, the color gradient shifts towards a slightly redder tone. This could indicate a subtle age gradient within the stellar populations or the presence of dust obscuration. The galaxy displays a smooth, featureless appearance, lacking any obvious spiral arms, dust lanes, or other distinct structural features. The overall shape is roughly elliptical, with an intermediate axis ratio, leaning more towards an elliptical shape than a cigar shape, indicating minimal rotational support. There's no apparent evidence of recent or ongoing major mergers or tidal interactions. Any disturbances appear minimal, suggesting a relatively quiescent evolutionary history. The galaxy's luminosity suggests that it is a mid-sized elliptical galaxy.
