The galaxy presents as an elongated, disk-shaped structure, indicative of a spiral or lenticular morphology viewed nearly edge-on. The central region exhibits a concentrated, brighter luminosity, suggestive of a prominent bulge. The bulge appears to be relatively smooth and rounded. The surrounding disk shows a gradual decrease in luminosity extending from the central bulge. Overall color gradients suggest a population of older stars and a relatively low star formation rate. No distinct spiral arm features are discernible given the near edge-on view, although there are hints of obscuring dust lanes. There is no evidence of ongoing major mergers or significant tidal disturbances. The morphology is likely of a smooth, rotating system, not undergoing any significant gravitational interactions.
