The galaxy presents as a roughly elliptical object with a bright, concentrated central bulge. The color profile indicates a gradient, transitioning from a brighter, bluer core to a more subdued and redder outer region.  No distinct spiral arm structures are immediately apparent. The overall morphology suggests a disk galaxy, likely with a significant spheroidal component. Faint, diffuse extensions may indicate tidal features or minor disturbances to the galaxy's structure. The texture of the galaxy does not appear perfectly smooth; there is a clumpy distribution of light in the outer regions which may indicate active star formation.
