The galaxy appears to be an intermediate morphology system, exhibiting characteristics of both elliptical and spiral galaxies. A dominant, smooth central bulge is observed with a relatively high concentration of older stars, indicated by the reddish hue. Fainter blue regions are asymmetrically distributed, suggesting ongoing star formation, though at a moderate rate.  The outer regions display subtle signs of tidal disturbances or interactions, potentially indicative of minor mergers or past gravitational interactions. The galaxy's overall shape is neither perfectly elliptical nor a well-defined spiral, falling somewhere in between, with an estimated physical radius of approximately 5 kpc. Evidence suggests that the galaxy's mass is around 10^9.7 solar masses.
