The galaxy appears to be elliptical in morphology, displaying a generally smooth and centrally concentrated light profile. There is no apparent spiral structure, disk, or significant dust lane visible. Its shape tends towards round, with only slight deviation towards an elongated form. The galaxy presents a yellowish-red hue, suggesting an older stellar population, and indicative of relatively low levels of ongoing star formation. There are no obvious signs of any major ongoing merger events or tidal disturbances in the immediate vicinity.
