The galaxy presents as a somewhat elliptical structure, with a major axis significantly longer than its minor axis. The light distribution appears relatively smooth and centrally concentrated. There's a notable color gradient, with the central region exhibiting a yellowish-white hue, possibly indicating an older stellar population and/or a higher concentration of dust. Moving outward from the center, the color shifts towards a slightly redder shade, implying a change in the stellar population or dust content in the outer regions. There's little evidence of distinct spiral arms or prominent star-forming regions. The overall morphology suggests a relatively evolved system, likely an early-type spiral or lenticular galaxy, viewed at an oblique angle. No obvious signs of recent major merger activity are observed, although some subtle asymmetries in the outer isophotes might suggest minor interactions. The galaxy appears relatively isolated within the observed field.
