The galaxy presents as a spiral type, viewed at a moderate inclination, with an approximate diameter of 7 kiloparsecs. A discernible disk structure is present, displaying faint, loosely wound spiral arms, indicative of ongoing star formation. The arms exhibit a mottled texture, possibly due to HII regions or young star clusters. A bright, concentrated central bulge dominates the galaxy's core, characterized by a yellowish hue, suggesting a population of older stars. There are minor disturbances within the galaxy, likely due to gravitational interactions. This may be the start of a merger event, but may also just be a passing gravitational disturbance. Overall, the galaxy exhibits properties consistent with a system actively forming stars, albeit with hints of past or ongoing interactions.
