The galaxy presents as an elliptical or lenticular type, appearing cigar-shaped with a central bulge that is noticeably brighter and more concentrated than its outer regions. The light distribution suggests a relatively smooth morphology, with little evidence of spiral arm structures or significant dust lanes. Color gradients are subtle, with the central bulge exhibiting a yellowish hue, possibly indicating an older stellar population. The outer regions show a slight shift towards redder colors, potentially due to the presence of evolved stars. There is no apparent indication of active star formation in the central region, based on the lack of bright blue regions associated with star-forming regions, suggesting a quiescent or passively evolving system. There are no signs of interactions or tidal disturbances, suggesting the galaxy has not undergone a recent major merger. Overall, the galaxy appears to be a relatively undisturbed and evolved system.
