The galaxy presents a somewhat irregular, disk-like morphology. Its light profile is centrally concentrated, with a yellowish hue suggesting an older stellar population dominating the central regions. A fainter, bluer halo surrounds this core, possibly indicating ongoing or recent star formation.  The disk exhibits some signs of minor disturbances, with a slight asymmetry in its shape.  There is a subtle hint of spiral structure, though it is not well-defined. Overall, the galaxy appears to be relatively massive and currently exhibits a modest rate of star formation.
