The galaxy presents as a singular, relatively smooth, and rounded structure. Its color profile is suggestive of an older stellar population, with a dominant yellowish-red hue across the entirety of the visible body. There are no easily discernible spiral arms or bar structures. Light distribution appears centrally concentrated, lacking in prominent features such as dust lanes or bright knots of star formation within the galaxy's body. There may be a slight elongation. Evidence suggests it is not currently undergoing any major merging events or significant tidal disruptions.
