The galaxy presents as a relatively smooth object with a slight elongation, appearing as an elliptical galaxy when viewed from our vantage point. It exhibits a prominent central bulge, which graduates into an extended halo of fainter luminosity. The light distribution suggests a higher concentration of older stellar populations in the core region. The galaxy's color appears to be generally redder, likely indicative of an evolved stellar population and lower ongoing star formation activity. There may be some minor internal disturbances that point toward a possible merger or a more complex gravitational interaction in the past. The overall appearance suggests a mature galaxy nearing the end of its active star-forming phase.