This galaxy appears to be an elliptical type, exhibiting a relatively smooth, featureless morphology. There is a distinct central bulge, characterized by a yellowish-orange hue, suggesting an older stellar population. The galaxy shows an overall rounded shape, though it is not perfectly circular. There is little evidence of spiral arms or significant dust lanes. The galaxy displays a concentrated luminosity profile. Overall the galaxy appears to be relatively isolated with no obvious signs of recent or ongoing merger activity. The galaxy exhibits low levels of star formation.
