The galaxy presents as a slightly elongated, disk-like structure with a smooth, centrally concentrated bulge. Its color profile exhibits a gradient, transitioning from a warmer, yellowish hue at the galactic center to cooler, bluer tones in the outer regions. A clear spiral arm structure is not evident, and no prominent dust lanes are observed. The overall light distribution suggests an older stellar population, particularly concentrated within the bulge, and a modest level of ongoing star formation in the disk region. The galaxy appears relatively undisturbed, with no significant signs of recent major mergers or tidal interactions. Its morphology aligns with an early-type spiral galaxy, possibly an Sa or Sb type, oriented at a significant inclination to our line of sight.
