This galaxy exhibits a generally smooth morphology, with a slightly elongated, cigar-shaped form. The central region displays a concentration of light, appearing yellowish, which suggests a population of older stars. Fainter blue regions can be observed towards the outer edges, potentially indicating some ongoing star formation. There is no apparent evidence of major merging activity or significant disturbances in its structure, although there may be some subtle irregularities. The overall appearance suggests a lenticular or possibly a spiral galaxy viewed at an inclined angle, but a more detailed analysis would be needed to confirm its classification.
