The galaxy presents as a moderately luminous object with a generally elliptical morphology. The central region exhibits a concentrated bulge, characterized by a yellowish hue, indicative of an older stellar population. Moving outward from the core, a more diffuse disk component is observed. This disk shows a bluer color profile, suggesting the presence of younger, hotter stars and ongoing star formation. There are subtle indications of spiral arm structures, though they appear somewhat disrupted or flocculent. Faint, redder patches are also visible in the outer regions, possibly indicative of dust lanes or regions of older stellar populations. Overall, the galaxy appears to be in a transition stage, possibly evolving from a spiral towards a lenticular morphology, or experiencing some interaction evidenced by morphological disturbances.
