The galaxy presents a generally smooth morphology, appearing elongated or cigar-shaped. It shows a bright, concentrated central bulge that transitions smoothly into a more diffuse, fainter surrounding disk. The color profile suggests a mixture of stellar populations, with the central bulge appearing more yellow, potentially indicating older, redder stars, while the outer regions exhibit a slightly bluer hue, which could indicate the presence of younger, bluer stars and some ongoing star formation. There's no obvious indication of strong spiral arm structure or a prominent dust lane; however, the image resolution is limited. There may be a slight disturbance visible on one side of the galaxy; it could be a minor interaction or a slight asymmetry in the disk. Overall, the galaxy appears to be a relatively massive, evolved system, possibly an early-type spiral or lenticular galaxy experiencing a low level of star formation.
