The observed galaxy exhibits a roughly elliptical morphology. A bright, concentrated central bulge is apparent, exhibiting a color profile that skews towards bluer wavelengths. Circumscribing the central region is a fainter, more extended disk structure. Indications of spiral arm structures are subtle, with only faint, diffuse features visible. The outer regions of the disk appear relatively smooth, suggesting a lack of prominent star-forming regions or significant dust lanes. Some irregularities are noted in the upper right quadrant of the galaxy, potentially suggestive of a minor disturbance, but this requires further investigation. The overall color profile suggests a relatively mature stellar population, although the bluer core could indicate recent or ongoing star formation in the central region.
