The galaxy presents as a centrally concentrated object with a relatively smooth morphology. There is little evidence of spiral arm structure or significant dust lanes. The color appears to be generally yellowish, suggestive of a population dominated by older stars. The galaxy appears roughly elliptical, with no major distortions or tidal features indicative of recent major mergers. There may be a slight deviation from perfect ellipticity suggesting minor disturbances, but these are not prominent. The galaxy appears to be an isolated system within the observed field. 
