The galaxy exhibits a generally smooth morphology, appearing largely featureless. Its shape is approximately round, although some slight elongation is evident. The color profile indicates a higher concentration of older stars, with a dominant yellowish-orange hue in the central region. No prominent spiral arms or bar structures are visible. There is no strong indication of active star formation, rather, it is dominated by older stellar populations. There is no evidence of major mergers or significant tidal disturbances. The galaxy is reasonably well-defined, with no signs of major disruption, but it appears to have a very small disk, or to be mostly smooth.
