The galaxy presents as a single, centrally concentrated object. Its morphology suggests a predominantly smooth structure, with minimal indication of spiral arms or prominent disk features. The color profile leans towards the redder end of the spectrum. There is an absence of significant dust lanes or patchy star formation regions visible at this resolution. Overall, this galaxy appears to be a relatively quiescent system with a substantial fraction of its stellar population potentially residing in older populations. There is a slight suggestion of a possible minor interaction or disturbance in its morphology, but it appears mostly undisturbed.
