The galaxy presents as an elongated structure, suggesting a shape that deviates from a perfect spheroid. Its light distribution is uneven; a bright, concentrated region is evident on one side, with a notable gradient in luminosity moving away from this central area. This brighter region exhibits a bluer hue, indicative of potentially younger stellar populations. 

The opposing end of the galaxy displays a more diffuse and reddish color profile. This could indicate a higher concentration of older stars, or possibly the presence of dust obscuring bluer light. There may be some minor structural disturbance given the asymmetric distribution of light and the elongated shape.
