The galaxy presents as a relatively small, well-defined elliptical or lenticular structure. It exhibits a smooth light distribution, with a concentrated central bulge that transitions into a fainter, extended disk. The disk component appears to be oriented nearly edge-on relative to our line of sight. The color gradient suggests the presence of an older stellar population within the bulge, indicated by a yellowish hue, with slightly bluer tones along the outer edges of the disk suggesting the presence of at least some younger stars. No distinct spiral arm structures or dust lanes are readily discernible. The galaxy appears relatively isolated with no obvious signs of recent mergers or tidal interactions.
