The galaxy presents as a moderately luminous, disk-shaped system oriented at a slight angle relative to our line of sight. A central bulge is clearly visible, exhibiting a yellowish hue, suggesting an older stellar population. Surrounding the bulge, a bluer disk component indicates more recent star formation. The disk appears somewhat disturbed, with hints of asymmetry. There's a suggestion of potential tidal features, indicative of gravitational interaction, albeit relatively minor. The galaxy's star formation rate appears low to moderate. Overall, the galaxy seems to be transitioning, possibly influenced by minor gravitational interactions.
