The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light distribution suggests a spheroidal shape, tending towards round rather than elongated. The core region exhibits a bright, yellowish-white color. The outer regions gradually fade in intensity and exhibit a slightly bluer hue compared to the core, transitioning towards a more diffuse profile. No distinct spiral arm structures or prominent dust lanes are discernible. There is no clear indication of ongoing major merging events or significant tidal disturbances in its immediate vicinity. The galaxy possesses an apparent moderate size, suggesting a substantial stellar population.
