The galaxy presents a distinct, elongated morphology, consistent with a likely edge-on spiral or lenticular classification. The central bulge exhibits a bright, concentrated luminosity with a yellowish hue, suggesting an older stellar population. Moving outward from the bulge, a fainter, bluer disk component is visible, indicating the presence of younger stars and possibly ongoing star formation regions. The disk appears thin and relatively smooth, showing a notable lack of prominent spiral arm structures or significant dust lane obscuration. The outer regions of the galaxy fade gradually into the background, with a very low surface brightness, indicating a diffuse halo. There are no visually apparent signs of major mergers or significant tidal interactions. The overall appearance suggests a quiescent galaxy with a relatively low star formation rate and an evolved stellar population.
