This galaxy appears to be a relatively smooth, elongated object, likely an elliptical galaxy or a lenticular galaxy viewed edge-on. It exhibits a central bulge that is brighter and more concentrated than the surrounding regions. There is little evidence of spiral arms or distinct features such as star-forming regions. The galaxy displays a color gradient, transitioning from a bluer hue on the outer edges to a redder hue towards the core. This color difference suggests that the galaxy has a higher proportion of younger stars in the outer regions and a higher proportion of older stars in the inner regions. The galaxy appears to be fairly isolated, with no other galaxies or tidal features immediately apparent in its vicinity. The overall shape and color distribution suggest an evolved system with a relatively low rate of ongoing star formation.
