The galaxy presents as an elliptical or lenticular system, exhibiting a centrally concentrated bulge that graduates smoothly into an extended disk. The overall structure appears relatively smooth, with little evidence of prominent spiral arms or patchy star formation regions. The color profile indicates an older stellar population, with the central bulge displaying a yellowish-orange hue, suggesting a higher concentration of evolved stars. The disk, while less distinct in color, shows a slightly bluer tint compared to the bulge, hinting at the presence of younger stars, although not in significant quantities. The galaxy appears to be elongated, with a length roughly twice its width. There is no immediately apparent sign of tidal disturbances, major mergers, or strong interactions with neighboring galaxies.
