The galaxy presents as a generally smooth, elongated structure with a prominent central bulge. It appears to be an elliptical galaxy, exhibiting a cigar-like shape. There's a noticeable color gradient from the core outwards. The core displays a yellowish hue, possibly indicative of an older stellar population, whereas the outer regions have a slightly bluer tint, though not strongly suggestive of recent star formation. There is little evidence of spiral arms or significant dust lanes. No obvious major mergers or tidal disturbances are observed, although there might be minor asymmetries or subtle disturbances present. Overall, the galaxy exhibits the characteristics of a relatively massive system, potentially on the red sequence, with a moderate star formation rate.
