The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy appears roughly elliptical in shape, although its isophotes may exhibit some slight deviations from perfect ellipticity. The galaxy's color is relatively uniform across its extent, appearing yellowish, suggestive of a relatively old stellar population. There are no distinct knots of star formation or bright blue regions visible in the galaxy's disk, lending further support to this classification. There are no signs of a major merger or significant tidal disturbances, although a subtle asymmetry could hint at a minor interaction. The galaxy's light profile appears to gradually fade into the background, suggesting a relatively well-defined boundary.
