The galaxy exhibits a smooth, elongated morphology. It appears as a single, centralized object with a radial gradient in surface brightness, peaking at the core. The shape suggests a possible elliptical classification, although a highly inclined spiral cannot be ruled out based on this image alone. The color profile is suggestive of an older stellar population, with a yellowish-orange hue dominating. There are no distinct spiral arms, dust lanes, or prominent star-forming regions visible. Evidence of any major merging events is absent. Slight asymmetry is observed, but could be internal to the galaxy. The light is centrally concentrated and gradually fades towards the edges.
