The galaxy appears as a single, relatively smooth object, exhibiting a yellowish central concentration of light that fades gradually into the surrounding space. The shape is generally round, with a slight elongation giving it an elliptical form. There is no obvious presence of spiral arms or distinct features typically associated with disk galaxies. Faint, diffuse light extends outwards from the central region, indicating a possible halo or envelope of stars. No signs of major mergers or significant tidal disturbances are apparent, although there may be a very slight asymmetry in the outer regions that could indicate a minor interaction. The overall colour suggests an older stellar population, consistent with a lower rate of star formation.
