The galaxy presents as a relatively compact, elliptical or lenticular structure. It exhibits a smooth, diffuse light distribution with a high degree of central concentration. There is no clear evidence of spiral arms, bars, or distinct features such as dust lanes or star-forming regions. The galaxy has an overall round appearance, showing a smooth luminosity gradient. There is no indication of ongoing major mergers or significant tidal disturbances, which would disrupt the overall symmetry and smoothness. The color is weighted towards the redder end of the spectrum, which may suggest an older stellar population, lower levels of current star formation, and/or internal dust reddening.
