The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular type. The overall shape appears elongated, leaning towards a cigar-like structure rather than a perfectly circular form. A bright central bulge is evident, surrounded by a less luminous, more diffuse halo. There is a subtle color gradient, with the central region exhibiting a yellow to orange hue, indicating an older stellar population, while the outer regions display a slightly bluer tint, which could indicate the presence of some younger stars. The overall light distribution seems relatively uniform, with no obvious spiral arms or strong dust lanes visible. There are no signs of any recent major merger events or significant tidal disturbances; any disturbances that exist are minor at best. Based on the size, it appears to be a reasonably massive galaxy. The low star formation rate is consistent with its morphology.
