The galaxy presents as a lenticular or early-type spiral, viewed at a high inclination. Its morphology appears generally smooth, with a bright, concentrated central bulge that dominates the visual appearance. The disk component, if present, is faint and tightly wound, contributing primarily to the overall elongated shape. The color profile indicates a relatively evolved stellar population, with a yellowish hue dominating the galaxy's central regions. There is a subtle gradient towards slightly bluer tones in the outer regions of the disk, suggesting the presence of some younger stars, although star formation activity appears subdued. The galaxy shows no clear evidence of spiral arms or significant dust lanes. The overall light distribution suggests that the galaxy's luminosity is dominated by older stars within the bulge and a relatively quiescent disk.
