This galaxy presents as an elongated, elliptical structure, exhibiting a smooth, rather than clumpy, morphology. Its color profile leans towards the redder end of the spectrum, suggesting a population of older stars. The galaxy appears relatively undisturbed, without any obvious signs of major mergers or tidal interactions. There is, however, a subtle hint of asymmetry or minor perturbation visible in the outer regions of the galaxy's disk. The shape is cigar-like, and the light is concentrated towards the center, gradually fading toward the edges. Based on the object's color, it is likely that it is a relatively massive system, with very little star formation present.