The galaxy presents as a predominantly smooth, elongated structure. Its overall shape can be described as cigar-shaped. The central region displays a high concentration of light, indicating a prominent galactic bulge. The color appears slightly redder in the central bulge, suggesting an older stellar population. Moving outwards from the core, the galaxy gradually fades, with a subtle color shift towards bluer hues in the outer regions. This suggests the presence of some younger stars on the periphery, although the extent of any active star formation appears to be limited. There appears to be no obvious spiral arm structure and it is not showing signs of a major ongoing merger event. Faint disturbances might be occuring but are not obviously visible. 
