The galaxy presents as a slightly elongated, centrally concentrated light source. The core region is luminous and appears relatively smooth, indicating a possible spheroidal morphology. A faint and diffuse disk structure might be present around the central bulge but is not clearly resolved in the image. The galaxy exhibits a blue hue, which could be indicative of ongoing star formation, even though the overall structure appears largely evolved. No prominent spiral arms or dust lanes are immediately visible. There may be a small, irregular object in the proximity of the galaxy which could be a dwarf galaxy that is interacting with the central galaxy. The color gradient shifts from a bluer core to somewhat redder outer regions, suggesting a radial variation in stellar populations, with younger, hotter stars being more concentrated towards the center. The overall structure suggests that the galaxy is neither a pure elliptical nor a well-defined spiral but potentially a lenticular galaxy or a spiral galaxy undergoing morphological transformation.
