The galaxy presents as a moderately bright, elliptical form. The color gradient suggests a relatively old stellar population with a dominant reddish hue in the central regions, transitioning to a slightly bluer periphery. The light is uniformly distributed across the galaxy suggesting a smooth morphology, which indicates minimal presence of spiral arms, dust lanes, or prominent star-forming regions. The galaxy appears to have an approximate effective radius of around 4 kpc. There may be a subtle asymmetry or minor disturbance in the shape, but overall structure indicates the galaxy is mostly undisturbed.