The galaxy presents as an elliptical or lenticular morphology. The overall light distribution appears smooth, with no readily discernible spiral arms or bar structures. A color gradient is visible; the central region exhibits a yellowish hue, transitioning to a redder color towards the outer regions. This suggests an older stellar population dominates the central region, with potentially younger, bluer stars residing further outwards, but this is subtle. The galaxy's shape is somewhat elongated, exhibiting an intermediate degree of ellipticity between a spherical and a cigar-like form. There are no obvious signs of major interactions or mergers, though a slight asymmetry could indicate minor disturbances or past tidal interactions. The galaxy's brightness profile suggests a centrally concentrated light distribution. The lack of clearly defined features indicates that this galaxy is likely undergoing a relatively low rate of star formation currently.
