The galaxy presents as a relatively compact structure, with a noticeable degree of ellipticity. Its overall color appears to be somewhat redder, suggesting an older stellar population. The light distribution within the galaxy seems fairly smooth, indicative of either a lack of prominent spiral arms or a more spheroidal morphology. There may be a very slight hint of disk-like structure, but further analysis is required to confirm. There appears to be very little evidence of on-going active star formation.
