The galaxy exhibits a generally elliptical morphology, with a noticeable elongation. The central region displays a high surface brightness, appearing as a bright, concentrated core. The light profile appears to fade gradually outwards from the center, suggesting a smooth distribution of stars with no prominent spiral arm structures visible. Color gradients indicate a relatively redder core, potentially indicative of an older stellar population, transitioning to slightly bluer hues in the outer regions. The overall smooth appearance, coupled with the observed color distribution, suggests that this may be a relatively evolved galaxy with a significant spheroidal component. There are no distinct features such as dust lanes or prominent star-forming regions easily discernible in this image.
