This galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge region with a distinct, nearly spherical shape. The light distribution suggests a generally older stellar population, with a yellow hue indicative of evolved stars. There is some indication of potential interaction or merging with a smaller object, possibly a dwarf galaxy, creating a minor disturbance or elongated morphology. No clear spiral arms or disk structures are visible. Overall, it seems to be a reasonably massive galaxy with a moderate rate of star formation.
