This galaxy appears to be an elliptical galaxy with a smooth profile, as evidenced by the lack of distinct spiral arms or prominent dust lanes. It exhibits a notably elongated, cigar-like shape. The central bulge is prominent and intensely luminous, suggesting a high concentration of stars. The galaxy appears to be relatively isolated with little or no signs of on-going major merging events or significant tidal disturbances. There appears to be a neighboring galaxy or object. Overall, the galaxy presents a relatively quiescent and evolved morphology, indicative of reduced star formation activity.
