The galaxy presents as an elongated, spindle-shaped structure, indicative of an edge-on spiral or lenticular galaxy. It exhibits a smooth, diffuse light distribution with a bright central bulge or core. The color profile suggests an older stellar population, with a yellowish hue dominating the central regions. Fainter, bluish extensions are visible at the periphery, potentially indicating the presence of younger, hotter stars within a faint galactic disk. No distinct spiral arms are discernible. There is no evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity. The morphology is largely undisturbed, suggesting a relatively isolated system that has undergone minimal recent interactions.
