The galaxy appears as a moderately inclined disk galaxy. It exhibits a centrally concentrated bulge, transitioning smoothly into a fainter, more diffuse disk. The color profile suggests a yellow-orange hue in the central region, possibly indicating an older stellar population. Moving outward from the center, there is a slight color shift towards redder tones, with hints of blue in the outer regions of the disk, possibly indicative of some star formation. The galaxy does not appear to show strong spiral arm structures, instead exhibiting a relatively smooth and featureless disk. There is no visible dust lane obscuring the galactic center. The overall morphology suggests a galaxy somewhere between an elliptical and spiral type, leaning towards a lenticular classification. There is no obvious evidence of recent major merger activity or significant tidal disturbances. The galaxy's apparent size is relatively small.
