The galaxy presents a somewhat amorphous morphology, appearing neither purely elliptical nor a well-defined spiral. Its structure is largely smooth, with a central, concentrated bulge that appears slightly elongated. There is a faint suggestion of a disk component, evidenced by a subtle flattening and extension along a particular axis, but it is not a prominent feature. The galaxy exhibits a blue hue, suggesting the presence of a younger stellar population and ongoing star formation. There is no distinct evidence of any major merging events or significant tidal disturbances, although some minor asymmetry might be present. Overall, the galaxy seems to be in a transition phase, potentially evolving from a more actively star-forming disk galaxy towards a more quiescent, bulge-dominated system.
