The galaxy presents a somewhat lenticular morphology with a distinct central bulge and a surrounding disk component. The bulge appears relatively smooth, exhibiting a slightly concentrated brightness profile. The disk is not sharply defined, showing a more diffuse and less structured appearance. There is some indication of disruption or tidal features, possibly faint extensions or asymmetries in the outer regions of the disk, suggesting a minor gravitational interaction or past merger event. The galaxy's color indices reveal a mix of stellar populations. The central bulge exhibits a redder hue, indicative of older, redder stars, while the disk shows bluer tones, suggesting the presence of younger, hotter stars and ongoing star formation. The overall star formation rate appears relatively low based on the weak blue color.
