This galaxy presents as an elongated structure, consistent with a disk galaxy viewed at a high inclination, potentially close to edge-on. The central region exhibits a concentrated luminosity, suggesting a prominent bulge. The color profile appears reddened in the bulge region, indicative of an older stellar population. The disk shows a more diffuse light distribution, with subtle hints of bluer regions which may denote areas of ongoing star formation, though the image resolution limits definitive identification of spiral arm structure. There is an indication of some form of disturbance in the morphology. The galaxy appears moderately luminous and relatively massive. The light profile implies this galaxy is in an evolved state, with limited recent star formation.
