This galaxy appears to be an elongated, cigar-shaped system, presenting itself nearly edge-on relative to our line of sight. The central region exhibits a concentrated luminosity with a yellowish hue, suggesting a relatively older stellar population. The galaxy's light profile seems smooth with no apparent spiral arm structure or prominent dust lanes visible. The overall form indicates a system with limited ongoing star formation within the main body, as evidenced by the lack of strong blue light. There are no obvious signs of a major ongoing merger, although some minor asymmetry at the edges might hint at tidal interactions.
