The galaxy presents as a moderately luminous, relatively compact object. Its overall morphology is largely smooth, with minimal discernible spiral arm structure or prominent dust lanes. The light distribution appears somewhat centrally concentrated, suggesting the presence of a bulge component, possibly a supermassive black hole in the center. There is a slight elongation to its shape, a deviation from perfect roundness. The galaxy appears relatively isolated, with no immediately obvious signs of tidal interactions or ongoing mergers with other galaxies, though minor disturbances cannot be ruled out. The color profile indicates a mixture of stellar populations, with a generally redder hue dominating, suggesting an older stellar population and potentially a lower ongoing star formation rate. Faint blue regions imply a small population of younger, hotter stars.
