The galaxy presents as a somewhat elongated object, its major axis extending noticeably further than its minor axis. There is a central, brighter concentration of light, suggesting a possible galactic nucleus or bulge.

The overall color profile appears to be dominated by redder hues, with some evidence of bluer, potentially younger stellar populations. The spatial distribution of these colors suggests some inhomogeneity within the galaxy. There appear to be traces of a disk like structure, but no distinct arms.

There may be some minor disturbances present, though nothing dramatic or prominent.
