The galaxy appears to be an elongated, cigar-shaped structure. Its central region displays a concentrated, luminous core that transitions into a softer, more diffuse halo. The color gradient suggests a redder hue in the nucleus, indicative of an older stellar population, possibly a substantial bulge. Extending outward from the central region, the galaxy exhibits a subtle blueish tint, hinting at areas of ongoing star formation within its outer regions. No clear spiral arms are apparent within the galaxy, although the slight asymmetry present hints at a potential tidal interaction or minor disturbance.
