The galaxy presents a primarily smooth morphology, with a high degree of central concentration. The shape is somewhat elongated, appearing more intermediate than purely round, with a hint of cigar-shaped ellipticity. There is no obvious indication of a major merger, though minor tidal disturbances or interactions cannot be entirely ruled out. The object appears to be an elliptical galaxy with relatively little active star formation. The color profile indicates a population of older, redder stars contributing to the overall luminosity.
