The galaxy presents a generally smooth morphology, with a central bulge that dominates the light emission. The bulge appears roughly spherical and exhibits a bright, concentrated luminosity profile, indicative of a high stellar density. Surrounding the bulge, a fainter, more diffuse disk is discernible. The disk is oriented at an angle relative to our line of sight, giving the galaxy an overall elliptical appearance. There is little evidence of well-defined spiral arm structure within the disk, and it appears relatively featureless. The color of the galaxy appears to redden from its core to its halo indicating that most star formation appears to be concentrated in the core. There is no obvious indication of any ongoing major merger events or strong tidal disturbances. Based on the morphological assessment, the galaxy is most likely to be an early-type spiral or lenticular galaxy.
