The galaxy presents as an elliptical morphology, exhibiting a generally smooth, concentrated light distribution. It appears quite round in shape. There is a strong central bulge, which indicates an older stellar population is likely present. The galaxy's overall color appears relatively red. This also suggests an older stellar population with lower ongoing star formation activity, which would cause the redder color index. The general lack of distinct spiral arms or obvious dust lanes corroborates the likelihood of it being an elliptical galaxy with a dominant bulge. No evidence of current major mergers or tidal disturbances can be seen.
