The galaxy presents as an elongated, disk-shaped structure viewed at a significant inclination. There is a distinct central bulge, exhibiting a yellowish hue, suggesting an older stellar population dominating this region. Extending outwards from the bulge, the disk shows a bluer color, indicating the presence of younger, hotter stars and ongoing star formation. The dust lanes are not very well defined in the image. The galaxy exhibits an overall smooth texture, with only subtle hints of spiral arm structure. It appears to be in a relatively undisturbed state, showing no obvious signs of major mergers or tidal interactions. The overall luminosity profile suggests a centrally concentrated morphology.
