The galaxy presents as a slender, elongated structure, indicative of a potentially edge-on spiral or a lenticular (S0) galaxy. The central bulge is a diffuse, yellowish hue, suggesting an older stellar population with reduced star formation activity in the nucleus. Moving outward from the central bulge, subtle color variations are observed. Faint blue tinges are visible along the outer edges, potentially tracing regions of ongoing, albeit relatively low, star formation within a disk component. The overall morphology suggests a relatively quiescent system, with little evidence of major mergers or significant tidal disturbances. The smooth, cigar-shaped appearance indicates a possible lack of significant spiral arm structure or prominent dust lanes that would otherwise disrupt the light distribution.
