The galaxy presents a largely smooth, elliptical morphology. It appears to be a relatively massive system exhibiting a central concentration of light, suggestive of an older stellar population. The overall color is slightly reddish, likely indicative of a lower rate of current star formation activity. The galaxy does not show evidence of strong spiral arm structure or significant tidal disturbances, implying a lack of recent major mergers. There may be some slight elongation or distortion of the galaxy's shape, but it is closer to round than to being cigar shaped.
