The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile.  The light is generally yellowish in color, with a slight reddening towards the outer regions.  The galaxy appears well-defined, with no obvious signs of significant tidal disturbances or ongoing major merging events.  The galaxy appears somewhat elongated.  There is no presence of a distinct disk component and no signs of strong spiral arm structures.  Based on these characteristics, the galaxy likely hosts an older stellar population and exhibits a relatively low star formation rate.
