The galaxy appears as a bright, slightly elongated object with a smooth, relatively featureless morphology. It seems to exhibit a single, concentrated central bulge and very little or no indication of spiral arms or a distinct disk structure. The galaxy is fairly symmetrical with no strong evidence of any ongoing major mergers or tidal disturbances. The color is biased towards redder wavelengths, implying an older stellar population and low levels of ongoing star formation activity. The lack of prominent dust lanes supports the interpretation of an evolved system nearing the end of its star forming life.
