The galaxy presents a generally smooth morphology, suggesting an elliptical or lenticular classification. The light profile appears centrally concentrated, with a gradual decrease in surface brightness outwards. There is a hint of a faint, diffuse halo surrounding the main body of the galaxy. The galaxy exhibits a slight elongation, indicating a possible deviation from a perfectly spherical shape. The color appears relatively uniform, with a reddish hue, which is consistent with an older stellar population and lower levels of ongoing star formation. There is no visual evidence of spiral arms, dust lanes, or other distinct features typically associated with spiral galaxies. Overall, the galaxy appears to be a relatively quiescent system.
