The galaxy appears as a centrally concentrated system with a relatively smooth morphology. It has a slightly elongated, prolate shape, resembling a cigar when viewed in this orientation. There is no clear evidence of a spiral arm structure or a prominent disk. The light profile suggests a dominant bulge component. The galaxy's color is primarily yellowish, implying a stellar population that is generally older and less actively forming stars, although there is a hint of a blue population mixed with this older light. There are no obvious signs of ongoing major mergers or significant tidal disturbances within the immediate vicinity of the galaxy.
