The galaxy presents a largely smooth morphology, with a high degree of central concentration. There is evidence of a disk structure. The object exhibits a moderate degree of roundness, trending towards an elliptical shape rather than a highly elongated or cigar-like form. The colour profile shows a redder hue, suggestive of an older stellar population and/or significant dust obscuration. There is no strong indication of ongoing major merging activity, though subtle disturbances cannot be ruled out.
