The galaxy presents as a lenticular or early-type spiral, with a dominant, relatively smooth bulge. Its overall shape appears somewhat elongated, approximately cigar-shaped. No distinct spiral arm structure is immediately apparent. The light distribution is centrally concentrated, fading gradually towards the outer regions of the galaxy. The color profile suggests an older stellar population, with a subtle reddish hue indicating a lack of significant ongoing star formation. The galaxy shows minimal signs of disturbance or interaction with other galaxies. Overall, it appears to be a relatively isolated and quiescent system.
