The galaxy presents as a relatively smooth, round object with an estimated effective radius of approximately 6.3 kpc. A slight asymmetry may be present, possibly indicative of minor tidal disturbances. The color profile appears to be relatively homogenous and the galaxy appears to be a redder object. There is no distinctive disk or spiral structure observed. There is no clear indication of a major ongoing merger. The galaxy's luminosity suggests it is a luminous object. Considering the estimated star formation rate, it appears to be a galaxy with moderate to low levels of star formation.
