The galaxy presents as a relatively compact object. It exhibits a central bulge that appears largely smooth and spheroidal, possibly indicating an older stellar population. The surrounding disk component displays some structure, with hints of spiral arms or irregular features extending from the central bulge. The color profile suggests active star formation regions, particularly in the disk, where we observe patches of bluer light. There is a slight asymmetry evident in the disk structure, with one side appearing somewhat more extended or disrupted than the other. This could indicate past or ongoing interactions with a smaller companion galaxy, or internal disturbances. Overall, the galaxy seems to be in an intermediate stage of evolution, exhibiting characteristics of both elliptical and spiral galaxies.
