The galaxy presents as a yellowish, elliptical-like structure. Its light distribution is relatively smooth and centrally concentrated, with no obvious spiral arm structures or strong dust lanes visible. It appears somewhat rounded, showing some deviation from a perfectly spherical shape. The galaxy's color suggests a population of older stars, indicating a likely low rate of ongoing star formation. There might be a faint, diffuse halo surrounding the main body of the galaxy, but it is not sharply defined. There is no clear evidence of any major merging events or significant tidal disturbances in its immediate vicinity.
