The galaxy appears to be a relatively smooth, somewhat elliptical galaxy with a dominant central bulge. The light distribution suggests a high degree of central concentration, typical of early-type galaxies. The color gradient is subtle, but the core seems slightly more yellow, possibly indicating an older stellar population within the bulge. There is little evidence of prominent spiral arms or significant dust lanes. The overall structure is largely undisturbed, showing no major signs of ongoing mergers, but there is a slight disturbance that may indicate a minor tidal interaction or past accretion event.
