The galaxy presents a mixed morphological profile, exhibiting both smooth and featured characteristics. The overall shape is somewhat rounded, though deviates slightly toward an intermediate form. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. The surrounding disc structure displays a bluish tint, indicative of ongoing star formation. Patches of redder regions are scattered within the disc, potentially marking areas of dust obscuration or older stellar populations. There's an indication of minor disturbances within the galaxy, and potentially a small merger. The overall luminosity is high, suggesting a relatively massive system with a moderately high star formation rate.
