The galaxy presents as a faint, somewhat elongated object. Its central region appears more luminous than the surrounding areas, suggesting a possible bulge or concentration of stars. The color distribution appears uneven, with the central region exhibiting a slightly redder hue compared to the bluer fringes on either side. This could be due to older stellar populations dominating the center, while younger, bluer stars are more prevalent in the outer regions. The edges of the galaxy appear diffuse and ill-defined, hinting at a possible disk structure or extended halo. There's some indication of slight disturbance or irregularity in the galaxy's shape, although further investigation would be needed to determine the nature of this feature. Overall, the galaxy's morphology suggests an intermediate stage of evolution.
