The galaxy presents as a single, relatively smooth object. It is slightly elliptical in shape, appearing more elongated than perfectly circular. There may be very faint disturbances in the galaxy's form, but they are not obvious. The color distribution is primarily a yellowish hue, indicating an older stellar population. There is a lack of blue color, suggesting a low rate of ongoing star formation. The galaxy appears to be relatively isolated, without any obvious signs of a major merger in progress, although a minor interaction or past merger cannot be ruled out.
