The galaxy presents a generally smooth, elliptical morphology. It appears elongated in shape, resembling a cigar when viewed from our perspective. The central region exhibits a pronounced bulge that is yellowish in color, potentially indicating an older stellar population. Surrounding the central bulge, there's a more diffuse halo or disk component exhibiting a bluish hue, which could be indicative of ongoing star formation. There appears to be no significant signs of disturbance or tidal features, suggesting that the galaxy has not undergone any major mergers recently.
