The galaxy presents as a relatively smooth object, elliptical in shape with a discernible core region. The light distribution suggests a concentration of older stars within the central bulge. The galaxy is elongated, appearing cigar-shaped rather than perfectly spherical. There may be evidence of minor disturbances in the galaxy's structure, however these are not well-defined or easily noticeable. Overall, the galaxy displays a moderate level of star formation activity. There is no indication of any major ongoing merger or significant tidal interactions.
