The galaxy appears as a relatively smooth, elliptical or lenticular object. There is little evidence of spiral arm structure or significant dust lanes. The light distribution suggests a centrally concentrated spheroid with a gradual decline in luminosity towards the edges. The morphology is predominantly smooth, with a high degree of roundness. There is a possible minor disturbance or interaction noticeable in the galaxy's profile, though the main body seems undisturbed. The color gradient suggests an older stellar population; this is indicated by the reddish hue. The galaxy appears to be a fairly massive system, undergoing modest levels of star formation. There is some evidence that the galaxy is not fully settled, possibly due to a past or ongoing minor interaction.
