The galaxy exhibits an overall elongated, cigar-like shape. Its structure appears relatively smooth with no clearly defined spiral arms or a central bulge. The color distribution shows a subtle gradient, with a slightly bluer hue towards the center and a redder, less intense color toward the outer edges, possibly indicating a central population of younger stars. There is no apparent evidence of active merging or major disturbances in its overall structure. The galaxy’s morphology suggests it might be a dwarf galaxy, possibly a dwarf elliptical or a lenticular type, with low levels of current star formation.
