This galaxy presents as a somewhat diffuse structure, appearing generally elliptical in shape, although the exact morphology is difficult to classify definitively. The light distribution suggests a central bulge region that is not exceptionally prominent, exhibiting a gradual decrease in luminosity towards the outer edges of the galaxy.  A bluer hue is observable within the galaxy, this suggests the presence of younger stars.  There is evidence of some disturbances of the galaxy body that could be the result of minor tidal interactions. The system seems to be relatively isolated, with no apparent major companion galaxies in close proximity.  Although there are some structural irregularities, the galaxy does not appear to be undergoing a major merger. Overall, this galaxy seems to be in a state of transition, potentially evolving from a more active star-forming phase to a more quiescent state.
