The galaxy presents as a slender, cigar-shaped structure, indicative of an edge-on spiral or lenticular morphology. A central bulge is visible, exhibiting a yellowish hue, possibly suggesting an older stellar population. Extending outward from the central bulge is a fainter disk component, displaying a bluish tint at its outer edges. The blue color may indicate the presence of younger, hotter stars and ongoing star formation. There is no significant dust lane apparent from this vantage point, although internal obscuration cannot be ruled out. The galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or tidal interactions. Overall, the galaxy possesses a moderate luminosity.
