The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a predominantly smooth morphology. It shows a lack of prominent spiral arms or distinct dust lanes. The color profile suggests a moderate population of older stars, contributing to the overall yellowish-white hue, with perhaps some regions of more recent star formation activity, subtly visible in the faint blue tinges surrounding the galactic center. The galaxy is nearly round in shape, indicating a low degree of rotational support, and no visual signs of significant tidal interactions or ongoing merger events are evident. The overall appearance suggests a relatively evolved and settled stellar population.
