The galaxy appears as a relatively smooth, elliptical-like structure with a high degree of central concentration. The light distribution suggests a spheroid-dominated system. The galaxy displays a color gradient, transitioning from a slightly bluer hue in its outer regions to a redder color towards the core. This color variation could indicate a radial difference in stellar population, with older, redder stars concentrated in the center and younger, bluer stars in the periphery. No distinct spiral arms or prominent dust lanes are visible within the galaxy's structure. There appears to be very little star formation occurring throughout the system, except for one small, bright knot of gas and dust on the edge of the galaxy, possibly indicative of a small, ongoing starburst region. The galaxy appears largely undisturbed, with no signs of major tidal interactions or recent merger events.
