The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits an elliptical morphology with a high degree of central condensation. There is a slight elongation in its shape, suggesting it is neither perfectly spherical nor a highly flattened disk. The overall color profile indicates a population of older stars, leaning towards redder hues. There is little evidence of spiral arms or significant dust lanes. Indications are that star formation is present, but not dominant in the galaxy. There is no clear evidence of any major ongoing merger activity or significant tidal disturbances. The observed features are broadly consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy with an intermediate projected size.
