The galaxy appears as a relatively compact object. Its light profile is generally smooth, suggesting an elliptical or lenticular morphology. The color is primarily yellow-orange, indicative of an older stellar population with fewer young, hot stars. There is a slight elongation in the galaxy's shape, but it is mostly round. No distinct spiral arm structure or prominent dust lanes are visible. There is no evidence of a major ongoing merger event, though there may be minor tidal disturbances. It seems the system is mostly settled. Given the color and morphology, star formation is likely suppressed or occurring at a low rate.
