The galaxy appears as an elongated, cigar-shaped structure. The light distribution suggests a concentration of older stellar populations towards the center, exhibiting a yellowish-white hue, likely composed of older stars. The outer regions display a bluer tint, which might indicate ongoing star formation or the presence of a younger stellar population. There is no obvious spiral structure discernible in this image. Instead, the galaxy appears relatively smooth, with hints of faint disk-like features. There are no strong signs of any major disturbances or interactions with other galaxies. The galaxy's overall morphology indicates a relatively evolved system, possibly transitioning towards a more spheroidal shape.
