The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. Its color index appears redder than typical spiral galaxies, suggesting an older stellar population and reduced ongoing star formation. The galaxy exhibits signs of a possible interaction or merger, with a disturbed morphology that suggests the presence of tidal features or a recent merger event. There are several distinct clumps of luminous material visible within the galaxy, possibly indicative of star clusters or regions of enhanced star formation triggered by the interaction. The galaxy is relatively massive.
