The galaxy presents as a slightly elongated, lenticular or early-type spiral morphology. The central bulge exhibits a concentrated, yellowish hue, suggestive of an older stellar population dominated by red giants. There appears to be an extended but faint disk surrounding the bulge, though distinct spiral arm structures are not readily discernible within the resolution of this image. The disk exhibits a bluer color, possibly indicating ongoing, albeit subdued, star formation activity. The overall smoothness of the galaxy implies a relatively settled state. The galaxy displays a slight tidal distortion, possibly indicative of past or ongoing minor interactions with neighboring galaxies.
