The galaxy presents as a generally elliptical structure with a prominent bulge. The central region exhibits a concentrated, bright, and somewhat amorphous appearance, suggesting a high density of stars. A disk-like structure is faintly discernible, extending outwards from the central bulge. The galaxy displays a relatively smooth morphology, but there appear to be subtle irregularities or disturbances in the outer regions of the disk, perhaps indicative of minor tidal interactions or ongoing accretion events. Color gradients suggest a distribution of stellar populations with a higher concentration of older, redder stars in the bulge, while the disk exhibits bluer hues, potentially indicating more recent star formation activity. It is a relatively large galaxy, with an apparent elongated form. Overall, the galaxy seems to be an intermediate stage between a pure elliptical and a spiral galaxy, exhibiting properties of both morphological types.
