The galaxy presents as a relatively smooth, elliptical structure with a discernible core. Its central region exhibits a distinct reddish hue, possibly indicative of an older stellar population and/or dust obscuration. A fainter, diffuse halo surrounds the core, exhibiting a bluer color. The overall shape appears more lenticular than perfectly spherical, leaning towards an in-between morphology. There is little evidence of spiral arms or significant ongoing star formation. The galaxy does not appear to be undergoing any major merging events or showing signs of significant tidal disturbances.
