The galaxy appears to be an intermediate spiral type, viewed at a moderate inclination. A distinct central bulge is present, exhibiting a bright, concentrated luminosity indicative of a high stellar density. Surrounding the bulge, a faint disk is discernible, though detailed spiral arm structures are not clearly resolved. The disk appears to be somewhat patchy and uneven in surface brightness, potentially suggesting ongoing or recent interactions. There is a faint blueish hue surrounding the central bulge suggesting the presence of younger stars. Faint tidal features or distortions seem apparent on the disk's periphery, though resolution limitations impede definitive classification. The galaxy exhibits a low degree of smoothness overall. Some evidence may point to a past minor merger event.
