The galaxy presents as a centrally concentrated object with a relatively smooth appearance. There is a distinct core region exhibiting a brighter, yellowish hue, suggesting a population of older stars. Emanating from the central region, a fainter, bluish extension is visible, indicating a possible tidal feature or plume of younger stars. The galaxy is largely elliptical in shape, appearing mostly round with a slight cigar shape. There are subtle hints of disrupted morphology. Overall, the galaxy appears relatively isolated, with no immediate signs of ongoing major mergers, though some minor disturbances cannot be ruled out. The estimated mass of the galaxy is relatively high, suggesting a substantial stellar population. Star formation appears to be suppressed.
