The galaxy presents as a relatively smooth object, with an elliptical morphology dominating the structure. The light distribution is centrally concentrated, with a radial decrease in intensity from the core. The color profile shows a general yellowish hue in the central region which appears to be consistent with a population of older stars, suggesting that the galaxy has largely exhausted its gas reserves.

There may be some slight irregularities in the overall shape, possibly indicative of minor past interactions or internal structures that are not fully resolved in this image. There appears to be a slightly redder, irregular region to the right of the galaxy's center, which may suggest a small region of ongoing or recent star formation or possibly an area of dust obscuration. However, the overall appearance strongly favors a passively evolving galaxy.